The galaxy presents a largely smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with a gradual decrease in brightness extending outwards from the core. The central region appears relatively featureless. There may be a faint, diffuse halo surrounding the main body of the galaxy. Color gradients are subtle, but a slightly bluer hue appears towards the outskirts, suggesting a weak presence of younger stellar populations or ongoing star formation activity in the outer regions. The overall structure indicates a high likelihood of being a spheroidal galaxy. Evidences suggest that this galaxy is isolated, without any signs of significant tidal disturbances or interactions with other galaxies in its immediate vicinity.
