The object presents as a compact galaxy, approximately circular in appearance. It appears to have a bright, concentrated central region which graduates into a fainter outer halo. The core exhibits a yellowish-white hue, which may be indicative of an older stellar population. 

There is some evidence of bluer regions within the galaxy, potentially indicating regions of more recent star formation. These regions appear to be somewhat patchy and are not evenly distributed throughout the galaxy.

There are subtle indications of disturbances or tidal features, notably a slight asymmetry or plume-like structure extending from one side of the core, hinting at a possible interaction or past merger event. However, these features are not prominent and could also be the result of internal processes.
