The galaxy presents as a relatively smooth, elliptical form. The core region exhibits high luminosity, indicating a concentration of stars and potentially an active galactic nucleus. Progressing outwards from the core, the luminosity gradually decreases. There appears to be a slight asymmetry in the outer regions. Some minor disturbance in the morphology indicates potential past interactions, however the galaxy remains largely undisturbed. Color gradients suggest varying stellar populations; the core appears more yellow/white possibly indicating older stars, while the outer regions exhibit a slightly blue hue possibly indicating star formation. The size is relatively compact, but appears very distant.