The galaxy presents as a centrally concentrated, elliptical-like structure. Its light profile appears smooth, with a high degree of central concentration. The core region is a bright yellowish-white, implying an older stellar population. Fainter, somewhat bluish arms extend outward from the center, but they are not well-defined. There is an absence of prominent dust lanes or distinct spiral arm structures. Overall, the galaxy appears to be relatively undisturbed, showing no clear evidence of recent major mergers or significant tidal interactions. There may be some degree of ongoing star formation, based on the hint of bluer light in the outer regions, though it appears to be relatively low. The galaxy has a moderate redshift. The galaxy exhibits a slight elongation, deviating marginally from perfect circularity.
