The galaxy presents a generally smooth and rounded morphology. There is a distinct central bulge that appears to be the brightest region of the galaxy. The overall color profile suggests an older stellar population, with a yellowish-red hue dominating. No prominent spiral arm structures are visible. There is no clear evidence of significant dust lanes or recent major mergers. The galaxy appears relatively undisturbed, with a high degree of symmetry. Some very minor irregularity may be present in the outer regions. The galaxy is relatively compact.
