The galaxy exhibits a morphology consistent with an elliptical galaxy or a lenticular galaxy with minimal disk structure. Its shape is primarily rounded, deviating only slightly from perfect circularity. The galaxy's color profile is dominated by redder wavelengths with a fainter blue profile, suggesting a population of older stars and a relative lack of ongoing, significant star formation. However, there are some regions that exhibit a higher proportion of blue, indicating the presence of star-forming regions. There is little evidence of substantial tidal disturbances or ongoing major mergers; however, the shape of the galaxy is not perfectly consistent.