The galaxy exhibits a generally smooth morphology, with a central, brighter region that gradually fades towards the outer edges. It displays a slightly elliptical shape, appearing more elongated than perfectly circular. There is a hint of a disk-like structure. The galaxy's light is predominantly yellowish-white in the center, possibly indicating an older stellar population. The faint outer regions seem to have more blue tint, which is characteristic of younger star clusters. There may be some minor disturbances or interactions happening which are causing this variation. Overall, the galaxy appears relatively undisturbed and is not undergoing any major merging events.
