The galaxy presents a roughly elliptical morphology, though significant light artifacts contaminate the visual assessment of its true shape. The core exhibits a concentrated, bright region, suggesting a relatively high stellar density. A fainter, more diffuse halo surrounds the core, extending further along the horizontal plane than vertically, suggestive of a flattened spheroidal structure. There is a hint of potential tidal features or distortions present, but the prominent artifacts prevent a clear identification. The central region appears to be predominantly blueish-white, which could indicate younger stellar populations or active galactic nucleus activity. The outer regions exhibit a reddish hue, suggesting older stellar populations. Overall, the galaxy appears to be generally isolated, with only vague hints of interactions or disturbances.
