The galaxy presents as a relatively smooth, elliptical structure. It appears nearly circular in projection. There is a concentrated central bulge exhibiting a yellowish hue, suggesting a population of older stars. The overall color gradient transitions to bluer hues towards the outer regions of the galaxy, implying some presence of younger stellar populations, but at a low rate. There is no indication of a prominent disk or spiral arms, nor any signs of ongoing major mergers or significant tidal disturbances. The galaxy appears to be a relatively undisturbed, evolved system with limited star formation activity.
