The galaxy presents as a relatively smooth, elliptical-like object with a slight elongation. It exhibits a centrally concentrated luminosity profile, with a gradual decrease in brightness towards the outer edges. The color appears generally uniform across the galaxy, trending towards the redder end of the spectrum. There's no obvious spiral arm structure or prominent dust lanes. Overall, the galaxy seems to be a fairly relaxed system, without any signs of major ongoing mergers or significant tidal disturbances, though some minor disturbance cannot be ruled out. The size is moderately compact, and based on its overall morphology, it likely consists mostly of older stellar populations with a relatively low rate of star formation.
