The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a somewhat elongated shape, with its major axis significantly longer than its minor axis. The galaxy's color profile suggests an older stellar population, with a redder hue dominant throughout its structure, especially towards the central bulge. There is no discernible spiral arm structure or significant dust lane presence within the visible spectrum. The light distribution appears relatively uniform, with a concentration towards the center. There is a possibility of minor gravitational interaction. Overall, it appears to be a passively evolving system, with a relatively low rate of star formation.
