The galaxy presents as an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The core of the galaxy is a bright, yellowish-white, indicating a population of older stars. Moving outward from the core, the light gradually diminishes, with a faint, elongated halo extending along a major axis. There is a slight suggestion of a subtle disk-like structure, although the galaxy remains largely spheroidal. No distinct spiral arms or dust lanes are discernible. There is no apparent evidence of any ongoing major mergers or significant tidal disturbances.
