The galaxy presents a generally smooth, elliptical morphology. Its core region exhibits a bright, concentrated luminosity, transitioning outward to a less intense, diffuse halo. Color gradients are discernible: the central region appears more yellow, suggestive of an older stellar population, while the outer regions show a bluer hue. Although the overall structure is smooth, subtle features potentially indicate the presence of a disk component or minor disturbances. No strong tidal tails or prominent merging features are evident; however, it is possible that there are some subtle disruptions. The galaxy is approximately 12 kpc across.