The galaxy presents an elliptical morphology, appearing somewhat cigar-shaped. The central bulge exhibits a yellowish-gold hue, suggesting an older stellar population. The outer regions of the galaxy display a more greenish tint, possibly indicating the presence of younger, hotter stars or ongoing star formation, although at an apparently low rate. The galaxy shows a smooth appearance, with no obvious spiral arm structure or significant dust lanes visible. There is a slight indication of tidal disturbance or a minor merger event in the galaxy's outer regions, but further investigation is needed to confirm this. Overall, the galaxy appears to be a relatively massive system.
