The galaxy presents a largely smooth and elliptical morphology. The central region displays a bright, concentrated core exhibiting a yellow-white color, indicative of an older stellar population. Moving outward from the core, the color profile shifts towards a redder hue, with the outer regions appearing more diffuse and less luminous. There is little evidence of distinct spiral arm structures or significant dust lanes. The galaxy appears relatively undisturbed with only minor irregularities in its overall shape. The overall spheroidal appearance suggests it is a fairly massive system with a relatively low star formation rate.
