The galaxy exhibits an elliptical morphology, presenting a smooth, concentrated light profile that gradually fades toward its periphery. It displays an intermediate ellipticity, appearing neither perfectly spherical nor highly elongated. The galaxy's core is characterized by a bright, concentrated luminosity. The overall color appears relatively red, suggesting a population dominated by older stars and a lower rate of on-going star formation. There is no apparent evidence of spiral arms or significant dust lanes. The galaxy appears relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions.
