The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, centrally concentrated morphology. The light distribution is characterized by a high degree of radial symmetry, with the isophotes appearing largely regular and elliptical. The central region is bright, indicative of a substantial stellar population density, likely dominated by older, evolved stars. The color is predominantly yellowish-red across the galaxy, suggesting a lack of significant ongoing star formation and a dominance of older stellar populations. There is very little evidence of spiral arm structure or a prominent disk. The galaxy is relatively isolated and appears undisturbed, showing no signs of tidal interactions or recent merger activity. The outer regions fade gradually into the background sky. There is a subtle flattening visible, suggesting it is not perfectly spherical. 
