The galaxy presents a generally smooth, elliptical morphology. It appears to be largely featureless, lacking prominent spiral arms or a distinct bar structure. The light distribution is centrally concentrated, with a bright core that diminishes gradually outwards. The color gradient suggests an older stellar population, with a yellowish-orange hue dominating the central regions, transitioning slightly to a bluer periphery, indicating possible recent, but minimal, star formation activity at its outskirts. The overall roundness suggests a classification closer to an E0 or E1 elliptical, showing minimal flattening. There is no visual evidence of ongoing major mergers or significant tidal disturbances in the immediate vicinity.
