The galaxy appears to be a relatively smooth, elliptical-like structure with a concentrated central bulge. There is a slight elongation, but it is mostly round in appearance. The color gradient suggests a stellar population primarily composed of older stars, indicated by the reddish-yellow hue in the central region. Fainter, blue-ish tinges on the outer edges could suggest the presence of some younger stellar populations, but are not very strong. No spiral arms or other distinct features are readily visible. The overall morphology indicates the galaxy is not undergoing any major merger events or significant tidal disturbances.
