The galaxy appears to be an elliptical type, with a relatively smooth and concentrated light profile. The central region exhibits a bright, reddish-orange hue, suggesting an older stellar population. Surrounding the core, the light diffuses outward, with a gradual decrease in intensity. There appears to be some mild disturbance to the symmetry of the galaxy, possibly resulting from a past merger. Overall, the galaxy seems to be relatively massive and exhibits little to no active star formation.
