Hi Greg,
In answer to your question, one of the standout galaxy groups in the Grus region is the IC 1459 group, which is dominated by the Elliptical or very mildly S0 (i.e. large bulge with a minimal or faint disk) morphology galaxy IC 1459.
This rather bright and easy group of galaxies is rarely imaged!
It needs a very large field.
I believe that Mr Sidonio made a good image of this group of galaxies with his previous imaging rig.
It is quite rich, for a galaxy group, and it has several members with peculiar morphologies.........
IC 5264 shows interesting signs of asymmetry in its dust distribution, but it is rarely imaged at high resolution.
Here is a composite of two different DSS images of IC 5264:
NGC 7418A is a challenging and low-surface-brightness galaxy of very strange appearance that has been modelled as being the product of an interaction or a merger between galaxies.
Here is the GALEX view of N7418A in the FUV and NUV
bands :
Here is a DSS composite (of R+J plates) from the Aladin database of DSS images:
NGC 7421 is a noticeably asymmetric spiral galaxy. There is an arm or arc on one side that has the appearance of being a bow shock, but there is no corresponding feature on the other side:
(The above is a blue photograph from the "NASA Atlas" of Sandage and Bedke. The asymmetry is less pronounced in red sensitive images.)
NGC 7418 is a bright and interesting spiral, which is relatively symmetric in the bright regions of its disk, however most extant images of NGC 7418 are shallow.
Here is an image of NGC 7418 from the survey OSUBSGS :
IC 5269A and IC 5269B are also interesting members of this galaxy group.
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It is hard to say how many faint galaxies may be lurking in this galaxy group, as very deep imaging of the IC 1459 group is virtually non-existent!
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cheers, the bad galaxy man