The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central region with a gradual decrease in luminosity towards its outer edges. There is a slight elongation in its shape, deviating from a perfect circular form. The color profile appears predominantly reddish-orange, suggesting an older stellar population, possibly with limited ongoing star formation. There are some faint hints of disturbances in the outer regions which may indicate minor interactions or past mergers with smaller galaxies. The overall morphology lacks distinct features such as spiral arms or a prominent disk.
