The galaxy presents as a single, relatively smooth object with a slightly elliptical morphology, exhibiting characteristics of an early-type galaxy. The core region shows a concentration of light with a reddish hue, potentially indicative of an older stellar population. This central concentration is surrounded by a more diffuse, yellowish-green halo. The lack of defined spiral arms or significant dust lanes suggests a quiescent star formation history, though the greenish tinge in the outer regions could point to some ongoing, albeit limited, star formation activity. There are no obvious signs of major mergers or significant tidal disturbances, although some minor irregularities may be present. The galaxy exhibits a moderate size. The apparent lack of significant structural features implies the galaxy is relatively evolved.
