The galaxy presents as a generally smooth, elliptical-like structure. It exhibits a concentrated central bulge that appears yellowish in color, suggesting a population of older stars. A faint, diffuse halo of greenish light surrounds the central region, potentially indicating some level of ongoing, albeit subdued, star formation. There is a very slight asymmetry to the shape, though no major disturbances or tidal features are visible. The overall morphology points towards a relatively quiescent system, with a high probability of being a non-merging galaxy.
