The galaxy presents as a relatively smooth, elliptical structure. The core exhibits a bright, concentrated luminosity, suggesting a high density of stars or an active galactic nucleus. Moving outward from the core, the luminosity gradually decreases, with the outer regions appearing more diffuse. There is a slight bluing in the galaxy's extended disk. The overall morphology indicates a system that is nearing the end of its star forming period. There are no obvious signs of major mergers or tidal disturbances, though there is minor disturbance.
