The galaxy presents as a moderately bright, elliptical-like object, exhibiting a smooth light distribution. The core is well-defined and relatively bright, with a diffuse glow extending outwards, fading into the background sky. The galaxy appears to be neither perfectly spherical nor highly elongated; its shape is somewhere in between. There is no obvious spiral structure, nor any prominent dust lanes or knots of star formation visible. The overall color suggests a population of older stars, with a slight bluer tinge in the central region. No signs of strong tidal interactions or disturbances are observed, suggesting that the galaxy is relatively isolated and undisturbed. The gradient of color suggests older populations of stars as you reach the outer edges of the galaxy.