The galaxy presents as a somewhat elliptical, although not perfectly round, structure. The central region exhibits a concentrated and bright yellowish hue, suggestive of an older stellar population. A diffuse, fainter halo surrounds the central region. There is a distinct, localized region of redder light on one side. There are no clearly defined spiral arms or bar structures visible. The overall morphology indicates a galaxy that is likely undergoing little to no major merging events.
