The galaxy appears to be elliptical or lenticular in morphology, displaying a smooth, relatively featureless structure. The light distribution suggests a high degree of central concentration, with a bright core. The galaxy exhibits a subtle color gradient, with the core trending towards a yellow-white hue, suggesting a population of older stars. The outer regions possess a slightly redder tint. There is no readily apparent disk structure, spiral arms, or any indications of ongoing major mergers or tidal disturbances. The overall shape is close to circular, with only a slight ellipticity visible.
