The galaxy presents a largely smooth, elliptical morphology with minimal discernible structure within the observed bands. The core region exhibits a high surface brightness and a yellowish-white coloration, indicating an older stellar population dominating the central bulge. A gradual decrease in surface brightness is observed moving outwards from the core, transitioning to a slightly redder hue in the outer regions. The isophotes appear generally circular, suggesting a low ellipticity. There are no visible signs of spiral arms, dust lanes, or ongoing major merger activity. Subtle asymmetries and minor disturbances are not entirely absent, suggesting a potentially complex or dynamic past, though these features are not immediately prominent within the available data. The overall appearance points towards a relatively massive galaxy, likely with a suppressed star formation rate.
