The galaxy presents as an elliptical-like morphology, elongated in shape. The central region exhibits a bright, concentrated core that fades smoothly towards the outer edges. The galaxy's color gradient suggests a population of older stars in the center, indicated by a slightly redder hue, shifting to a bluer tone in the outskirts, which hints at possible, albeit limited, ongoing star formation. No distinct spiral arms or prominent dust lanes are visible. The overall structure appears relatively smooth, showing minimal signs of recent major merger events or significant tidal disturbances.
