The galaxy presents as a relatively smooth, elliptical-like structure with a centrally concentrated luminosity profile. It exhibits a high degree of circular symmetry, with minimal deviation from a perfect spheroid. There is no apparent spiral arm structure or prominent dust lanes visible. The color is generally consistent across the galaxy, with a subtle redder hue in the central region compared to the outer edges. There is no evidence of ongoing major merging activity or significant tidal disturbances. The object appears relatively undisturbed and quiescent in nature. The galaxy seems to be a fairly massive system, indicative of a evolved stellar population and potentially low star formation rate.
