The galaxy appears to be a relatively smooth, elliptical-like structure. Its central region exhibits a high degree of luminosity, appearing nearly spherical, with a noticeable decrease in intensity towards its outer edges. There's a slight elongation of the galaxy along one axis. Faint disturbances or tidal features are suspected in the galaxy's outskirts. The colour profile suggests a concentration of older stellar populations, indicated by the yellow to reddish hue of the galaxy body. Limited presence of prominent dust lanes or distinct spiral arm structures indicates an earlier stage of morphological evolution.