The galaxy presents a largely smooth, elliptical morphology. The core region exhibits a concentrated, bright luminosity, with a yellowish hue suggesting an older stellar population. There is a gradual decline in surface brightness from the core outwards, leading to a diffuse halo. Though largely smooth, there are faint hints of structure or asymmetry in the outer regions, but not enough to qualify it as a spiral or barred spiral. There are some slight irregularities that point to possible minor disturbances. The overall color profile indicates a possible red-sequence galaxy.
