The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that appears yellowish-white, indicating a significant population of older stars. The galaxy's light profile suggests it is fairly centrally concentrated. The outer regions are less luminous and display a subtle blueish hue, suggestive of some recent star formation activity. The galaxy shows a slight elongation, appearing more "in-between" round and cigar-shaped. There is no obvious evidence of a major ongoing merger. Based on the colors, star formation is present but not dominating the features of the galaxy. 
