The galaxy presents as a generally smooth, elliptical-like structure. It is concentrated in the center, with the intensity of the light decreasing gradually towards the edges. The core exhibits a yellowish, golden hue, which could be indicative of an older stellar population. There are faint traces of blue, but overall there is a lack of significant spiral arm structures or dust lanes. The overall shape is close to circular in appearance. There is no evidence of any significant merging activity, however the slight distortions may suggest minor disturbances.
