The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a centrally concentrated bulge, appearing nearly spherical. The light profile appears to decrease smoothly from the core outwards, with no distinct spiral arm features immediately discernible. The color gradient suggests a predominantly older stellar population throughout the galaxy, with slightly bluer hues in the outer regions indicating some recent or ongoing star formation, although at a low rate. There is no significant evidence of tidal disturbances or major merging events.
