The galaxy presents as a flattened, elliptical form, viewed at a moderate inclination. A distinct central bulge is apparent, characterized by a bright, concentrated luminosity suggesting a high stellar density and potentially an older stellar population. Surrounding the bulge is a disk-like structure exhibiting subtle color variations, possibly indicative of differing stellar populations or dust lanes. The overall smoothness of the galaxy suggests a relatively evolved system with a dominant spheroidal component. There is some distortion, hinting at a possible tidal interaction in the past, but it could also be due to internal processes. The absence of strong spiral arm features reinforces the classification as an early-type galaxy. The colors seem to suggest a relatively low star formation rate. 
