This galaxy appears to be a luminous elliptical galaxy, exhibiting a smooth, concentrated morphology. The central region displays a bright, yellowish hue, suggesting a population of older stars. Moving outward from the core, the light gradually fades, and a subtle transition towards redder tones is observed. The overall shape of the galaxy is somewhat elongated, but largely regular. There is no readily discernible spiral structure or significant dust lane. Marginal disturbances are present with minor asymmetries in the outer regions, which could possibly indicate tidal interactions, although a major merger seems unlikely.
