The galaxy presents as a somewhat smooth object, although not entirely featureless. It exhibits a moderate degree of elongation, appearing more cigar-shaped than circular. There is a hint of internal structure, possibly indicating a disk-like component, but the resolution is insufficient to definitively confirm this. The color gradient suggests a central bulge region that is more yellow/orange, possibly indicative of an older stellar population. The outer regions are slightly bluer, implying ongoing star formation. There seems to be a merger present that is causing a tail of dust and stars to be ejected. There's a minor disturbance possibly causing minor tidal features. Overall, the galaxy appears to be undergoing a period of interaction or disturbance.
