The galaxy presents a generally smooth morphology, displaying characteristics consistent with an early-type galaxy. The light distribution indicates a centrally concentrated structure, with a gradual decrease in intensity outwards. There is a subtle color gradient observed within the galaxy, transitioning from a redder core region to bluer, less prominent outer regions. This hints at possible variations in stellar population age and composition, with older, redder stars likely dominating the central region.

There is little evidence of spiral arm structures or significant dust lanes within the galaxy. The galaxy shape is not perfectly round, presenting a slightly elongated shape. There may be some minor asymmetries or subtle distortions in the galaxy's outer regions, which could be indicative of past or ongoing minor interactions or mergers. Overall, the galaxy appears relatively undisturbed.
