The galaxy presents as a fairly smooth, elliptical or lenticular structure, with a prominent central bulge. The luminosity appears concentrated towards the core, suggesting a high stellar density in this region. The overall color profile indicates a population of older stars, with a redder hue dominating the galaxy's disk and bulge, implying minimal ongoing star formation. A faint, diffuse halo may be present, though its extent is difficult to discern against the background. No spiral arm structure is visible, nor are there obvious signs of tidal disruption or interaction with other galaxies, suggesting it is not currently undergoing a major merging event. The shape is tending towards rounder, as opposed to being highly elongated. Overall, the galaxy exhibits characteristics typical of a passively evolving system.