The galaxy presents as a somewhat diffuse, centrally concentrated luminous object. The overall shape appears to be largely spheroidal, with a discernible though not perfectly circular morphology. The central region exhibits a brighter intensity, gradually fading towards the outer edges. There appears to be some degree of perturbation or tidal disturbance in the galactic structure, presenting as a knot of light adjacent to the central light of the main galaxy, indicative of a possible ongoing or recent interaction, such as a merger with a smaller galactic body. The primary light emitted by the galaxy is weighted toward the longer wavelengths suggesting a population of older stars.
