The galaxy presents as a relatively smooth, elliptical-like morphology. It exhibits a concentrated central bulge, indicated by a bright and compact core. There is an apparent absence of spiral arms or prominent disk-like features. The galaxy appears somewhat rounded. There is no visual evidence of any ongoing major merging events or significant tidal disturbances. The color profile suggests a dominant population of older stars, with the galaxy appearing more red than blue. Overall, the galaxy displays characteristics consistent with a massive, evolved system with a low star formation rate.
