The galaxy presents as a relatively bright, lenticular object, exhibiting a smooth, centrally concentrated morphology. Its overall color index suggests an older stellar population, predominantly yellowish-orange, especially in the core region. There is evidence of a slightly more diffuse halo or disk, exhibiting a bluer color. The axial ratio indicates that the galaxy is viewed at a moderate inclination. There appears to be a region of star formation activity to the right. The observed characteristics are consistent with a massive galaxy that is either undergoing a star formation event or merging with another galaxy.
