The galaxy presents a largely smooth, elliptical morphology. It appears nearly circular, with a slight elongation visible along what appears to be its major axis. The core region exhibits a bright, concentrated luminosity, suggesting a high stellar density or possibly AGN activity. The color gradient suggests a somewhat older stellar population, particularly towards the central bulge which appears reddish or golden in tone. Fainter, bluish hues are seen in the outer regions, perhaps indicating some residual, low-level star formation, but overall the galaxy appears relatively quiescent. There's no clear evidence of spiral arms or significant dust lanes. The general structure appears undisturbed; no major tidal features or signs of a recent major merger are readily visible. Subtle irregularities or minor disturbances might be present in the outer halo but at this resolution, it's challenging to confirm.
