The galaxy presents as a flattened, elliptical morphology. The central region exhibits a high concentration of light, appearing smooth and yellowish-white, likely indicative of an older stellar population. Moving outwards from the center, the light distribution becomes less concentrated, and appears a slightly bluer hue. There is a slight hint of a disk-like structure. The overall structure displays a moderate degree of disturbance, possibly suggesting a past or ongoing minor interaction or merger event. There does not seem to be significant evidence of major merging activity.
