The galaxy exhibits a morphology consistent with an elliptical type. It presents a smooth, centrally concentrated luminosity profile, suggestive of an older stellar population. The overall shape appears somewhat flattened, deviating slightly from a perfectly spherical distribution. There is a slight color gradient from the center to the outer regions, where the edges appear to have a slightly bluer hue. This subtle color variation could indicate the presence of some star formation activity or a younger stellar population in the galaxy's outskirts, although the dominant color is redder, which could be consistent with low star formation rates and an evolved stellar population. There may be minor disturbances in the galaxy's structure possibly caused by minor disturbances, although the galaxy itself shows a relatively undisturbed structure. There appears to be a hint of disk-like structure.
