The galaxy presents as a slightly elongated, elliptical structure. It exhibits a smooth, centrally concentrated light profile, with a bright core that gradually fades into the outer regions. There is a marginal asymmetry noted in the outer isophotes. The color appears to be predominantly white and light blue, suggesting a relatively older stellar population with a moderate ongoing star formation rate. No distinct spiral arms or prominent dust lanes are discernible. There is no evidence of a major merger event occurring with any other galaxies.
