The galaxy presents as a relatively smooth, centrally concentrated object. Its overall form approximates an elliptical shape, with a gradual decrease in luminosity observed moving outwards from the core. There may be a subtle disk-like feature. Color gradients are present, with a slightly bluer hue in the outer regions, transitioning to a more yellow-white color towards the central bulge. There is no strong evidence of spiral arm structures, bar features, or significant tidal disturbances. The galaxy appears relatively isolated and non-interacting, although there may be minor asymmetries in the luminosity distribution indicating minor past interactions. Overall, the galaxy is likely a relatively massive elliptical or lenticular galaxy, with a moderate rate of star formation.
