The galaxy presents as a moderately bright, relatively small, and somewhat diffuse object. It exhibits a flattened, disk-like morphology, although the disk is not sharply defined. The color appears somewhat blue, suggesting the presence of a moderate population of younger, hotter stars and ongoing star formation, but this blue hue is not dominant. The galaxy's shape is elliptical. There is a faint, diffuse halo surrounding the main body of the galaxy, suggesting a smoother stellar distribution. There appears to be little to no evidence of strong spiral arm structure or a prominent central bulge. Minor disturbances appear in the morphology, such as clumps of starlight. It does not show any signs of a major ongoing merger, although there could be minor interactions.
