The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated, yellowish core, suggesting an older stellar population dominating the central region. The isophotes appear mostly regular and symmetric. There is a slight ellipticity. No spiral arms or dust lanes are apparent. The galaxy lacks any obvious signs of active star formation, with a smooth transition in color from the core outwards. The object is likely a high mass galaxy with a relatively low star formation rate. There is no indication of a major merger.
