The galaxy presents a smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with a gradual decrease in brightness towards the outer regions. The galaxy appears relatively rounded, with a slight elongation. There is no apparent evidence of spiral arm structures or prominent dust lanes. The color distribution is dominated by redder hues, particularly towards the core, suggestive of an older stellar population. There might be a very faint, diffuse halo surrounding the main body, but its presence is subtle. No significant merger activity or tidal disturbances are readily observable. The overall impression is that of a relatively quiescent, evolved galaxy.
