The galaxy presents a generally smooth, elliptical morphology. There is a suggestion of a more flattened shape, tending towards oblate rather than perfectly spherical. The core exhibits a relatively high surface brightness, surrounded by a more diffuse halo of fainter luminosity. The light distribution appears primarily smooth, with no visually discernible spiral arm structures or prominent dust lanes. There are some disturbances possibly from a minor merger. Overall, the galaxy seems to be undergoing active star formation.
