The galaxy appears as a centrally concentrated object, generally elliptical in shape. There is a smooth, diffuse halo extending outwards from a bright core. The galaxy has a yellow hue with some of the central regions being slightly more white. There is no indication of distinct spiral arms or prominent dust lanes; instead, the light appears to be evenly distributed and consistent with an older stellar population. Based on its morphology, it is likely that star formation activity is relatively low within the galaxy. There is no evidence of any ongoing merger events or strong tidal disturbances affecting the galaxy's structure.
