The galaxy presents as a somewhat diffuse, centrally concentrated object. It displays a generally elliptical morphology, appearing more smooth than structured. The central region is dominated by a bright, yellow-tinged core, potentially indicating a concentration of older stars or dust obscuration. There are hints of bluer regions further out from the nucleus, likely representing areas of more active star formation. The overall structure suggests a galaxy that is either elliptical, or perhaps a spiral system viewed at an angle that obscures its spiral arms. There is some indication of disturbances in the galactic morphology.
