This galaxy presents a generally smooth, elliptical morphology. The central bulge appears bright and concentrated, indicating a high stellar density within the core region. The galaxy exhibits a color gradient, shifting from a more yellow-white hue in the central bulge to slightly redder tones in the outer regions of the halo. There's minimal evidence of spiral arm structures or significant dust lanes, suggesting a likely classification as an early-type galaxy. The roundness of the galaxy suggests it is nearly face-on, and no signs of any major ongoing merger are present. There is a feature visible on the bottom right, which appears to be a tidal tail or small, nearby object. The color profile and overall structure indicates that the galaxy possesses a well-evolved stellar population, with a relatively low current star formation rate.
