The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears largely elliptical, displaying a gradual decline in luminosity from a bright, compact core outward. There is a hint of a faint, diffuse disk-like structure, but no prominent spiral arms or bar features are visible.

The color profile suggests a population of older stars, with the central bulge appearing somewhat bluer than the outer regions. There is no clear indication of recent or ongoing major star formation events. Based on its overall appearance, the object is likely a relatively massive galaxy with a low specific star formation rate. There is no obvious evidence of strong tidal interactions or recent merging activity.
