The galaxy presents as a relatively smooth, elliptical-like structure. Its light profile suggests a centrally concentrated bulge, with luminosity decreasing gradually towards the outer edges. The color distribution is not uniform; the central region exhibits a yellowish hue, potentially indicating an older stellar population. The outer regions appear somewhat bluer, hinting at the presence of younger stars, though these are not clearly resolved. There is no apparent spiral arm structure. The galaxy appears somewhat elongated, lacking perfect circular symmetry, and there is no obvious sign of ongoing major mergers or significant tidal disturbances in the immediate vicinity, though the subtle asymmetry suggests the possibility of a past interaction.
