The galaxy presents a generally smooth, elliptical morphology with hints of internal structure. A bright, concentrated central bulge dominates the galaxy's luminosity profile. Surrounding the bulge, a more diffuse halo is observed, gradually fading into the background sky. There appears to be a slight asymmetry in the outer regions, possibly indicating minor gravitational interactions or tidal disturbances with a past or present companion. The color gradient suggests the core population is older. The presence of bluer regions indicates ongoing or recent star formation. The galaxy exhibits a moderate degree of roundness, appearing neither perfectly spherical nor highly elongated.
