The galaxy presents as a smooth, centrally concentrated object with an elliptical morphology. It appears to be a relatively undisturbed system. The color profile suggests a dominant population of older stars, exhibiting a redder hue towards the center that gradually transitions to a slightly bluer color in the outer regions. There are no obvious signs of significant spiral arm structure or ongoing major merging activity, though a subtle asymmetry hints at a possible minor interaction or internal disturbance. The galaxy appears to be quite massive and exhibits a moderate level of star formation. Overall, this galaxy seems to be a mature system, characterized by a well-established structure and a gradual decline in star formation activity.
