The galaxy presents as a relatively smooth, centrally concentrated object. The overall morphology appears elliptical, with a deviation from perfect sphericity. There is a slight elongation observed. Its color is a yellowish hue suggesting a dominant population of older stars and a reduced rate of on-going star formation. No prominent spiral arms or distinct features are visible, though there may be subtle irregularities in the light distribution. It does not appear to be undergoing a major merger or significant tidal disruption, but it could be experiencing minor disturbances, or past minor disturbances, due to it's morphology. The galaxy is estimated to have a substantial stellar mass.