The galaxy presents as a relatively smooth, elliptical-like structure with an apparent disk, though the disk is not sharply defined. There is a color gradient, with the central region appearing yellower, transitioning to a more greenish hue in the outer regions of the disk. The central bulge is prominent, appearing as a concentration of older stellar populations. Faint redder extensions or possible tidal features are very subtly visible, suggesting a possibility of prior minor interactions or mergers. The overall morphology suggests an intermediate elliptical galaxy at a substantial distance from the observer. The galaxy is not perfectly round, appearing slightly elongated. There is no obvious sign of a major ongoing merger or significant star formation.
