The galaxy presents as a single, centrally concentrated luminous object. It is observed as a generally smooth distribution of light, appearing largely spheroidal. The object exhibits a radial color gradient, appearing bluer toward the outer edges and redder towards the core. There is no obvious presence of spiral arm structures or a distinct galactic disk, however the outer edges are slightly irregular, perhaps due to an ongoing minor gravitational interaction. The central region is intensely bright, suggesting a high concentration of stars or the possible presence of an active galactic nucleus. The morphology appears consistent with an elliptical galaxy undergoing some limited star formation.
