The galaxy presents as a relatively smooth, centrally concentrated object with an elliptical morphology. The core region exhibits a yellowish-orange hue, potentially indicative of an older stellar population. The outer regions display a bluish tint, which could suggest the presence of younger stars or ongoing star formation, albeit at a modest rate. The galaxy's shape is elongated, with a moderate cigar-shaped appearance. There's a lack of any distinct spiral arm structure or obvious signs of a major merger event in progress. Minor disturbances may be present in the outskirts of the galaxy.
