The galaxy presents as a relatively smooth object with a well-defined elliptical morphology. Its overall color is a blend of yellow and red, indicative of an older stellar population, particularly concentrated towards the central bulge, although some recent star formation can be observed. The galaxy exhibits a distinct central bulge region that gradually fades into a more diffuse halo. The major axis appears to be significantly longer than the minor axis, which gives it an elongated appearance. There is a slight suggestion of a disk-like structure, based on its oval form. The axial ratio indicates it is relatively inclined, which could contribute to the observed elliptical shape. There are hints of what appear to be slight disturbances, likely due to minor mergers.
