The galaxy presents as a centrally concentrated, elliptical-like structure. It exhibits a smooth, relatively featureless morphology with a high degree of radial symmetry. The light distribution suggests a spheroidal component is dominant, with the intensity peaking towards the core. There is a slight elongation, with the galaxy's shape falling somewhere between round and cigar-shaped, but leaning closer to being round. There's an indication of a slight color gradient, with the central region appearing more yellow, suggestive of an older stellar population, while the outer regions possess a slightly bluer hue. No signs of spiral arms, bars, or prominent dust lanes are apparent in this image. The galaxy appears undisturbed, without obvious signs of a recent or ongoing major merger event, though minor disturbances cannot be ruled out.
