The galaxy presents as a roughly elliptical structure with a concentrated central bulge. The light distribution appears relatively smooth, suggesting a lack of significant spiral arms or prominent dust lanes. The color gradient transitions from a bluer hue on the galaxy's periphery to a whiter, more neutral color toward the center, which could indicate a higher concentration of older stellar populations in the core. There appears to be some minor asymmetry. Overall, the galaxy gives the impression of a mature system with moderate star formation activity. There is a small amount of disturbance visible, but it isn't a major aspect of the galaxy's appearance.
