The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge, with a diffuse halo extending outwards. The color profile suggests a dominant population of older stars, with a possible presence of younger stars in the central region as indicated by a slightly bluer hue there. There is no discernible spiral structure or prominent dust lanes. The galaxy appears relatively isolated, with no obvious signs of tidal disturbances or ongoing major merger activity.
