The galaxy presents as a somewhat elliptical structure, appearing largely smooth with a concentrated central bulge. The color profile suggests a population of older stars, with a yellowish-orange hue dominating. There are subtle hints of bluer regions, possibly indicative of recent or ongoing star formation. The overall light distribution appears relatively even with a slight elongation, exhibiting no strong spiral arm features or prominent dust lanes discernable. It seems the galaxy may have undergone some form of past interaction or disturbance, as it does not appear completely relaxed. However, the disturbance is not significant as it doesn't show large tidal tails or obvious signs of a major merger.
