The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge, transitioning into a more diffuse halo. The color profile suggests a population of older stars, as indicated by its reddish-yellow hue. There is no evidence of spiral arms or significant dust lanes within the galaxy. The overall morphology is consistent with an early-type galaxy undergoing little to no active star formation. The galaxy does not appear to be interacting with any other galaxies or showing signs of tidal disturbances.
