The galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth, concentrated light profile with a slight elongation. The central bulge region is bright and appears yellowish-orange in color, suggesting a population of older stars. Fainter, diffuse light extends outwards from the bulge, forming a halo-like structure. There is some slight evidence of a disk component. The galaxy is not perfectly spherical but appears somewhat flattened, which, along with its color and estimated size, suggest the galaxy has ceased or is no longer actively forming stars. There are no distinct spiral arm structures or dust lanes visible in the image. Based on its morphology, the galaxy may have undergone or be in the process of merging with another, smaller galaxy.
