The galaxy presents as a fairly smooth, elliptical structure. A central bulge dominates the light profile, appearing a yellow-orange hue, suggesting an older stellar population. The outer regions of the galaxy are less concentrated and exhibit a bluer tint, indicative of the presence of younger stars or ongoing star formation, although not particularly vigorous. The galaxy is elongated, exhibiting a cigar-like shape, but overall shows a moderate degree of symmetry. There is no discernible dust lane or prominent spiral arm structure. The overall appearance suggests that the galaxy has undergone some past interaction or disturbance, but it currently does not appear to be undergoing a major merger event.
