The galaxy presents as a centrally concentrated object, exhibiting a generally smooth morphology. It appears largely elliptical in shape, with only subtle deviations from perfect circularity. The light distribution suggests a dominant bulge component, characterized by a yellowish hue, which gradually fades towards the outer regions. There is little indication of distinct spiral arm structures or prominent dust lanes. Some slight distortions or irregularities may be present at the periphery, but overall, the galaxy appears relatively undisturbed. The color profile implies a stellar population that is somewhat evolved, potentially indicating a low current star formation rate.
