The galaxy presents as a roughly elliptical, moderately luminous object. Its central region exhibits a high degree of concentration, appearing significantly brighter and more intensely colored towards the core. The color gradient suggests a population of older stars dominating the central bulge. Moving outward from the center, the galaxy's luminosity gradually decreases, forming a more diffuse halo. The morphology suggests the galaxy is relatively undisturbed, showing no signs of major mergers or tidal interactions, and the general appearance is smooth and lacks any distinct spiral arm structures. There's a slight elongation to the galaxy's shape, but it is generally round.
