The galaxy appears as a single, fairly smooth object with a slightly elliptical morphology. It exhibits a concentrated central region. The color gradient suggests a radial profile, with the core appearing more yellow, transitioning to red towards the outer regions, possibly indicating an aging stellar population or dust obscuration in the central regions. No distinct spiral arms or prominent dust lanes are discernible. There may be minor disturbances, but overall it does not appear to be undergoing major merger activity.
