The galaxy presents as a relatively smooth, elliptical morphology. Its core is luminous, displaying a yellow-orange hue, indicative of an older stellar population. The light appears concentrated towards the center, suggesting a significant bulge component.

The outer regions of the galaxy exhibit a gradual decline in brightness. There are subtle color variations within the galaxy, with hints of bluer tones in the outer fringes. However, these features are faint, which suggests that the fraction of younger stars is relatively low in these regions. The galaxy appears largely undisturbed, with no obvious signs of tidal tails or major mergers in progress. There are some slight irregularities, however, that indicate that a minor merger or interaction with a small object may have occurred.

Overall, this galaxy seems to be an evolved system, with a dominance of older stars and a generally quiescent star formation rate.
