The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated, bright central bulge that appears reddish-white in color, suggesting a population of older, redder stars. Surrounding the bulge is a more diffuse halo. This halo shows a faint bluish tint, hinting at the presence of some younger, bluer stars and possibly ongoing star formation, though at a low rate. The galaxy's overall structure appears relatively undisturbed with no clear signs of ongoing major merger activity or significant tidal distortions. The galaxy's shape appears fairly regular, neither perfectly spherical nor significantly elongated. There may be some minor irregularities in the outer regions of the halo, possibly indicative of a minor interaction or accretion event in the galaxy's past. Overall, this galaxy appears to be a relatively evolved system.
