The galaxy presents as a centrally concentrated elliptical galaxy, exhibiting a smooth, featureless morphology. The core of the galaxy displays a bright, yellowish-white hue, suggesting a population of older stars. Radially outward from the core, the galaxy appears as a more diffuse halo, fading gradually into the background. The elongation of the galaxy is subtle, indicating a close to circular projected shape. There is no discernible evidence of spiral arms, dust lanes, or active star-forming regions within this galaxy. It is primarily a passively evolving system. No signs of major tidal disturbances, mergers or interacting companions are noted.
