The galaxy presents as a generally smooth, single structure. Its shape appears largely elliptical or lenticular, with a high degree of central concentration. The overall color is yellowish, suggesting a population of older stars. A slight hint of blue or green tint towards the outer regions indicates some ongoing, albeit limited, star formation activity. There are no clearly discernible spiral arms or significant dust lanes visible. There is no visible indication of any major ongoing merger or significant tidal disturbance. The light distribution suggests a relatively quiescent galaxy, most likely a massive system with a moderate rate of star formation.
