The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a concentration of light, appearing yellowish-white, suggesting a population of older stars. Fainter, bluer hues surround the central bulge, possibly indicating the presence of some younger stars. The overall shape is elongated, and without distinct spiral arm structures. There is no evidence of significant ongoing mergers or major disturbances to its structure. The galaxy is not perfectly round, instead showing some ellipticity.
