The galaxy appears to be an elliptical galaxy, presenting a relatively smooth, featureless profile. It exhibits a distinct elongation, appearing cigar-shaped. The light distribution is centrally concentrated with a yellowish hue in the core, indicative of an older stellar population. Fainter, bluer light surrounds the core in a diffuse halo, which may indicate some ongoing, though limited, star formation. There is no visual evidence of spiral arms or significant dust lanes. No signs of tidal tails, distortions, or other indications of recent major merger activity are apparent, suggesting this is a relatively undisturbed system.
