The galaxy presents as a centrally concentrated object with a diffuse, smooth morphology. The core region appears luminous, potentially indicative of a high concentration of stars or an active galactic nucleus. The light distribution diminishes gradually from the core outwards, lacking any distinct spiral arm features or strong bar structure. There appears to be an absence of significant dust lanes or prominent star-forming regions within the visible extent of the galaxy. The overall shape seems close to elliptical with some possible asymmetry and there are no signs of a recent merger or strong tidal interactions. The color of the galaxy is slightly blue in the center and then reddish in the edges, which suggests that star formation occurred more recently in the center than in the edges.
