The galaxy presents a largely smooth, elliptical morphology. It appears relatively undisturbed, showing no strong evidence of recent major mergers or tidal interactions. The light is concentrated towards the center, indicating a prominent bulge. The color gradient suggests a population of older stars, with a redder hue dominating the overall light. There is a slight hint of a disk-like structure, but the dominant impression is that of a spheroidal system. Faint outer regions extend beyond the brighter central part. The galaxy displays intermediate roundness.
