The galaxy presents as a centrally concentrated object, exhibiting a smooth, somewhat elliptical morphology. There is a lack of any prominent spiral arm structure or distinct features, indicating it is likely an early-type galaxy. Color gradients within the galaxy show a radial trend, with a slightly bluer core transitioning to redder outer regions. The overall color suggests a stellar population dominated by older stars with limited ongoing star formation. There is a subtle indication of a tidal tail on the top right side of the galaxy, which could indicate past or current merger activity.
