The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that transitions into a more diffuse halo. The color profile indicates a redder core region, potentially indicative of an older stellar population, which gradually becomes bluer in the outer regions, suggesting more recent star formation activity, although limited. The overall structure appears undisturbed, with no obvious signs of tidal interactions or major mergers. The shape is largely round with minimal elongation. Based on the observed color and morphology, this galaxy likely hosts a significant stellar mass.
