The galaxy presents a moderately luminous profile, appearing as a relatively small, diffuse object. The central region exhibits a concentrated, brighter core. This core is surrounded by a less defined, extended halo of fainter light. There is evidence of some structural features, possibly indicative of spiral arms or tidal disturbances, but these are not sharply defined, with one side appearing more disturbed than the other. Overall, the galaxy appears somewhat irregular in shape. There may be ongoing, low-level star formation activity.
