The galaxy appears as a lenticular or possibly elliptical type. It displays a centrally concentrated bulge which fades into a smooth and diffuse halo, with no obvious spiral arm structure. Its overall shape is elongated, approximately cigar-shaped. The light distribution appears relatively even, suggesting a lack of significant recent star formation. There is no evidence of ongoing mergers or tidal disturbances, though the possibility of a past minor interaction cannot be entirely excluded.
