The galaxy presents as a single, luminous object with a generally elliptical morphology. It appears smooth, without any prominent spiral arm structures or significant dust lanes visible at this resolution. There is a bright central bulge which appears yellowish, suggesting an older stellar population dominating the core. The galaxy appears to gradually fade in intensity towards its outer regions, transitioning to a reddish hue. There is a hint of a faint, blueish halo extending to one side, which could indicate some recent, minor interaction or star formation activity. No strong signs of ongoing mergers or major disturbances are apparent in the galaxy's overall structure.
