The galaxy presents as a generally smooth, centrally concentrated object. It exhibits a roughly elliptical morphology. There is a slight asymmetry in the light distribution, potentially indicating minor gravitational interactions. The color profile suggests a relatively older stellar population, with a central yellow-white hue indicative of evolved stars. There is also a slight redder region on one edge of the galaxy. The overall apparent size suggests a moderate physical extent. No distinct spiral arms or prominent dust lanes are discernible at this resolution, further supporting a classification toward early-type galaxies.
