The galaxy presents as a largely smooth, centrally concentrated elliptical morphology. The central region exhibits a bright, yellowish hue, suggesting a significant population of older stars. Moving outward from the core, the galaxy fades into a more diffuse, bluish halo, possibly indicating a younger stellar population or some degree of ongoing star formation, albeit at a lower rate. There's no distinct evidence of spiral arms or significant tidal disturbances, however a slight asymmetry in the outer halo on one side could suggest a minor interaction. The overall roundness of the galaxy is suggestive of an early-type system.
