The galaxy exhibits a predominantly smooth morphology. It appears generally elliptical in shape, though it is not perfectly round. There is a suggestion of a slight elongation, but it could also be a distortion. No distinct spiral arms or bar structures are apparent upon visual inspection. The light distribution is concentrated towards the center of the galaxy, with a gradual decrease in intensity outwards. The galaxy's color profile seems to be fairly homogenous across its extent, showing minimal color variation or patchiness. There is no clear evidence of tidal tails, plumes, or other strong indicators of recent major mergers. However, there might be a slight distortion or irregularity in the outer regions that could suggest a minor interaction or disturbance. 
