The galaxy presents as a centrally concentrated, elliptical-like structure. It exhibits a smooth, diffuse morphology, lacking the distinct spiral arm features often observed in disk galaxies. There's a discernible color gradient, with the core appearing predominantly yellowish-red, suggesting an older stellar population. The outer regions display a faint blue hue, possibly indicative of some younger stars or ongoing, albeit limited, star formation. The galaxy appears relatively undisturbed, showing no obvious signs of a recent major merger or tidal interactions. There are no prominent dust lanes or other distinct features interrupting the smoothness of the overall structure. The object appears approximately round, although it could be described as slightly elongated. Overall, the galaxy seems to be a relatively quiescent system, primarily composed of older stars, with only a low level of current star formation activity.
