The galaxy presents a largely smooth and elliptical morphology. It exhibits a concentrated central bulge that appears bright and luminous. The surrounding galactic halo displays a more diffuse and faint light profile. The overall color suggests a population of older stars, with a general lack of prominent spiral arms or significant dust lanes. The galaxy appears to be relatively undisturbed, without obvious signs of ongoing major mergers or tidal disruptions. The system appears to be relatively isolated, as there are no other galaxies nearby to be interacting with. There may be evidence of faint, diffuse extended structures.
