The galaxy presents as a roughly elliptical, smooth object. There is little to no disk structure visible. The light profile appears concentrated towards the center, with a gradual decrease in brightness further from the core. The galaxy exhibits a yellow/orange hue in the central regions which fades into a slightly redder tone further out. This color may suggest an older stellar population dominating the galaxy's composition and comparatively low amounts of recent star formation. There does not appear to be any evidence of spiral arms or significant dust lanes. The overall morphology suggests an early-type galaxy. There is no visual evidence of any major merger events.
