The galaxy presents as a relatively smooth, elliptical-like structure. It is a faint and diffuse object, exhibiting a central bulge that is more luminous than its outer regions. The galaxy has a somewhat circular morphology, appearing mostly undisturbed. There is a lack of any obvious spiral arm structure or prominent dust lanes. Color gradients suggest a population of older stars, especially toward the center, with a possible, albeit difficult to discern, younger stellar population in the outer regions, giving them a slightly bluer appearance. Overall, the galaxy seems to be in a relatively quiescent state, without any major ongoing mergers or tidal disturbances.
