The galaxy presents as a relatively smooth and centralized object, potentially an elliptical or lenticular galaxy. The central bulge is bright and exhibits a yellowish hue, suggesting an older stellar population. Fainter, bluer light extends outwards in a flattened disk-like structure. There are no clear spiral arms or significant dust lanes visible, supporting the smooth classification. The overall shape appears close to an intermediary, with a slight elongation. No obvious signs of recent or ongoing major mergers are detected. The overall color profile suggests that star formation is limited.
