The galaxy presents as an elliptical morphology, appearing largely smooth with a dominant central bulge. The color gradient indicates a relatively old stellar population, characterized by a yellowish-red hue. The object exhibits a modest effective radius, suggesting a compact structure. There are no readily discernible spiral arms or distinct dust lanes. The overall appearance indicates a galaxy in a relatively quiescent state, with low to moderate star formation activity. There does not appear to be evidence of any major ongoing merging events, but there could be minor disturbances present. The elongated appearance suggests it is not perfectly round, but instead somewhere in between round and cigar-shaped.
