The galaxy appears to be a relatively smooth, elliptical type. Its overall shape is quite round, exhibiting very little deviation from circular symmetry. The light distribution seems largely uniform across its surface, with a gradual decrease in brightness from the center towards the outer edges. There is no evidence of spiral arms, a distinct galactic disk, or significant dust lanes. The galaxy's core exhibits a bright, concentrated glow which may represent a supermassive black hole. There is no evidence of any merging activity or major tidal disturbances, however there appears to be a slight asymmetry which suggests the possibility of a minor past interaction. The color appears to be generally reddish, indicating an older stellar population and a lack of ongoing star formation.
