The galaxy appears to be a relatively smooth and centrally concentrated object. It exhibits a generally elliptical morphology, appearing more "in between" than perfectly round or cigar-shaped. There is no prominent disk or spiral structure visible, suggesting it may be an elliptical galaxy or a lenticular galaxy seen face-on. The galaxy's light distribution is generally even, with a gradual fall-off in intensity from the core to the outer regions. There is no strong evidence of ongoing merging activity or major disturbances in its structure, although minor disturbances cannot be ruled out at this resolution. The color of the galaxy is on the redder end of the spectrum.