The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There is an indication of a slight disk-like structure that is visible around the bulge. The galaxy appears to be generally spheroidal but not perfectly round, with a somewhat elongated form. It shows a colour gradient, with the central region exhibiting a warmer, yellower hue, suggesting an older stellar population. The outer regions show bluer hues, indicative of younger stars or star formation. There is no obvious evidence of spiral arms or significant merging activity. The galaxy appears relatively undisturbed morphologically.
