The galaxy presents a largely smooth, elliptical morphology. The light distribution appears fairly uniform, with a slightly brighter central region indicating a possible nucleus. There is little evidence of distinct spiral arms or significant dust lanes. The galaxy appears somewhat rounded in shape, and there does not seem to be any signs of any major mergers or tidal disturbances. It exhibits a color gradient, with the core appearing slightly more yellow than the outer regions. This color difference could suggest older stellar populations concentrated in the central region. Overall, this galaxy appears to be a relatively undisturbed, evolved system.
