The galaxy presents a smooth, elliptical morphology. Its color profile indicates a predominantly older stellar population with a concentration of light in the yellow-red bands towards the core and a slightly bluer hue at the extremities. The overall shape is elongated, but not excessively so, indicating a moderate degree of ellipticity. No distinct spiral arm structures or significant dust lanes are visible. The galaxy appears relatively undisturbed, showing no evidence of major ongoing mergers or tidal interactions. 
