The galaxy presents as a primarily smooth, centrally concentrated object. It exhibits a roughly elliptical morphology, with a high degree of central concentration gradually diminishing in brightness towards the outer regions. The core appears luminous with a slightly yellow-white hue, which is indicative of a high concentration of older stars. The outer regions display a bluer tint, suggesting the presence of some younger stars. There may be a subtle indication of a disk-like structure, however it could also be a spheroidal shape. No distinct spiral arms are observable. There may be a slight irregularity on one side, suggesting a minor disturbance, but no major morphological distortions or signs of an active merger are apparent.
