The galaxy exhibits an elliptical morphology, though some features suggest a possible disk-like structure or past interaction. The overall light distribution is concentrated towards the center, indicating a prominent bulge. The colors are indicative of intermediate to old stellar populations, with the central regions appearing more red, possibly due to a higher concentration of older stars and/or dust obscuration. There's a slight color gradient moving outwards, where colors shift slightly bluer, indicating younger stellar populations are more prominent at the galactic edges or arms. The galaxy shows no signs of major ongoing mergers, though minor disturbances in shape could hint at past tidal interactions or smaller accretion events.
