The galaxy exhibits a generally smooth morphology, with a near-circular shape. The central region is relatively bright, suggesting a concentration of stellar mass and/or active galactic nucleus activity. A slight extension or minor disturbance is visible along one side of the galaxy. This could potentially indicate a tidal interaction with a smaller companion galaxy. The color of the galaxy is relatively uniform, suggestive of an older stellar population or significant dust obscuration, or strong emission lines dominating the spectrum. Overall, the galaxy appears to be a relatively undisturbed system, though some minor interaction might be present.
