The galaxy presents as a moderately luminous object, exhibiting a generally elliptical morphology. The light is concentrated towards a bright, seemingly unresolved nucleus, indicating a potentially significant central mass concentration. A surrounding, more diffuse halo appears to fade outwards from the central region. There are no obvious spiral arm structures or dust lanes visible in the galaxy; it possesses a rather smooth appearance. The color indices suggest a population of older stars are dominant, with a possible small fraction of young stars. There is no noticeable morphological disruption or tidal features, suggesting the galaxy is relatively undisturbed and not currently undergoing any major mergers.
