The galaxy presents as a centrally concentrated object with a smooth, largely featureless morphology. Its overall shape is elliptical, appearing mostly round. The light distribution indicates a prominent bulge component, with the majority of the galaxy's luminosity concentrated within the central region. There is a lack of discernible spiral arm structure or significant dust lanes. The galaxy exhibits a yellowish hue, suggestive of an older stellar population and relatively low levels of on-going star formation, consistent with a passively evolving system. There is no obvious evidence of any major mergers or tidal disturbances.
