The galaxy presents as a relatively smooth, luminous object. It appears roughly circular in projection, exhibiting a high degree of radial symmetry. The light distribution is concentrated towards the center, with a gradual decrease in surface brightness towards the outer regions, suggesting minimal spiral arm structure. There is a faint, diffuse glow in the surrounding area, with no evidence of tidal tails or significant morphological disturbances, indicating it is not presently undergoing a major merger. No distinct disk-like feature is apparent. A slight elongation is possibly discernable.
