The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology is primarily elliptical, appearing mostly round, although a slight elongation is discernible along one axis. The galaxy exhibits a luminosity profile that gradually decreases from the core outwards, lacking prominent spiral arm structures or dust lanes. It displays a yellowish hue, suggestive of an older stellar population with reduced ongoing star formation. There is no clear evidence of significant tidal disturbances or ongoing mergers in the immediate vicinity. It is a fairly massive galaxy, with a good amount of older stars.
