The galaxy presents as a luminous, elliptical morphology. Its core appears smooth, with a concentrated central bulge that emits strongly across the observed color bands, suggesting an older stellar population. The galaxy exhibits a relatively high degree of symmetry. The overall color is consistent with a evolved stellar population, though there are subtle color gradients within the galactic structure. The galaxy's light profile is gently declining, and the isophotes show a smooth, elliptical form. Based on the observed characteristics, it is likely to be a galaxy with ongoing star formation. The lack of apparent spiral arms or other features, suggests a relatively quiescent galaxy.
