The galaxy presents as a moderately bright, centrally concentrated object. Its overall morphology appears elliptical, exhibiting a smooth, diffuse luminosity profile without discernible spiral arm structures. The core region displays high luminosity, gradually decreasing towards the outer edges of the galaxy, suggesting an older stellar population. The isophotes are generally elliptical, with a moderate degree of ellipticity, and the galaxy appears relatively undisturbed, lacking strong tidal features or evidence of recent major mergers, although there is a potential tidal tail or plume on one side. Color indices suggest a redder population. Overall, the galaxy appears to be a relatively quiescent, mature system.
