The galaxy presents a largely smooth morphology, appearing elliptical in shape, although it is not perfectly round. There is a concentrated central bulge that emanates light across the yellow-orange spectrum, with fainter and more diffuse luminosity extending outwards. The outer regions exhibit a gradual decline in brightness, suggesting a lack of distinct spiral arms or features. There are hints of a disk-like structure, but it is poorly defined. The color profile indicates a population of older stars within the central bulge, while the outskirts appear somewhat bluer, suggesting the presence of a younger stellar population, but overall low levels of star formation. There is no visible evidence of tidal disturbances or recent mergers.