The galaxy presents a morphology dominated by a smooth, centrally concentrated component. It appears as a yellowish, elliptical-like form. There is some visual evidence of a potential disk, seen as a subtle, extended and slightly blue-tinted structure, possibly indicating ongoing star formation. The main body exhibits a higher concentration of older stars, suggested by its yellow-red hue. Possible signs of gravitational disturbance are visible in the surrounding area and may indicate a relatively late-stage merger event. Overall, the galaxy exhibits properties that might point towards a late-type spiral or an early-type elliptical undergoing a merger event.
