The object presents as a generally smooth, elliptical galaxy with a concentrated central bulge. The galaxy exhibits a subtle color gradient, with the core appearing a yellowish hue suggestive of an older stellar population. Moving outward from the core, the color gradually shifts to a slightly bluer tone indicating possible ongoing, yet limited, star formation within the galactic disc. The overall morphology suggests a relatively evolved system, likely a lenticular or early-type spiral galaxy viewed close to face-on. No strong tidal features or evidence of major merger activity are apparent; however, a minor asymmetry in the outer halo hints at potential past interactions or accretion events. The light distribution is fairly symmetric.
