The galaxy presents as a relatively smooth, centrally concentrated object with a generally elliptical morphology. The galaxy exhibits a bright central bulge that seems to be comprised of older stars. There is a subtle color gradient; the core is somewhat yellow, with the outer regions transitioning to a redder hue.  No spiral arm structure is visible. There appear to be no significant tidal features or indications of ongoing major mergers. The object appears to be isolated in this field of view. The light distribution suggests the galaxy is not perfectly spherical, possessing a slight elongation.
