The galaxy presents as a generally smooth, elliptical object. It exhibits a concentrated central bulge, which appears a warmer hue, suggesting a population of older stars. Moving outward from the core, the light appears to gradually fade. The outer regions exhibit a slightly bluer tint relative to the core, potentially indicating the presence of younger stellar populations or ongoing star formation, albeit at a low rate. The galaxy appears elongated, with an axial ratio deviating noticeably from a perfect circle. There is no clear indication of spiral arm structure, and no obvious tidal features or major disturbances are visible. A minor asymmetry can be seen at the bottom region of the galaxy. The galaxy's overall structure points towards a relatively evolved system, possibly an early-type spiral with a significant bulge, or potentially an elliptical undergoing very limited recent star formation.
