The galaxy appears as a single, relatively indistinct, luminous entity. The central region presents a yellowish-white hue, suggesting a significant population of older stars. Fainter reddish patches are visible along the periphery, indicating regions where star formation may be occurring, or regions with significant dust extinction. There is a slight asymmetry in the overall light distribution, potentially indicative of a minor interaction or disturbance. While largely elliptical in overall form, deviations from perfect symmetry are present. Based on the diffuse light surrounding the core, this is likely a relatively massive galaxy.
