The galaxy presents as a concentrated, elliptical-like structure with a smooth, diffuse light profile. It is largely devoid of prominent spiral arms or distinct features typically associated with disk galaxies. The light distribution is centrally concentrated, with brightness decreasing gradually toward the edges of the galaxy. The overall color appears to be a yellowish-white, suggesting a population of older stars with a relatively low rate of ongoing star formation. There is no evidence of significant dust lanes or active star-forming regions within the galaxy. Morphologically, it appears to be a relatively undisturbed system.
