The galaxy presents as a centrally concentrated, elliptical-like structure. The light profile appears smooth with a relatively high degree of symmetry, indicating a likely spheroid morphology. The color appears to be yellowish. There are no obvious spiral arm features and no significant dust lanes.

Based on color, the galaxy's stellar population is likely dominated by older stars, suggesting a relatively low current star formation rate. There's no evidence of tidal tails or strong morphological distortions, and the colors are consistent with a mature galaxy without ongoing major mergers. There is a slightly brighter concentration of light in the core. Overall, the galaxy appears as a relatively undisturbed, evolved system.
