The galaxy appears as a centrally concentrated object with a largely smooth morphology. It exhibits a near-circular shape and a lack of discernible spiral arm structures or significant dust lanes. There's no evidence of a recent major merger event in the galaxy's morphology, nor any apparent tidal tails or other major disturbances. The color profile suggests a population of older stars, with a slight color gradient from the center outwards. Star formation appears to be occurring at a low rate. The galaxy's light distribution follows a smooth profile, consistent with an elliptical galaxy.
