The galaxy presents as a luminous, elliptical structure with a smooth, centrally concentrated morphology. The core region exhibits a yellowish hue, likely indicating an older stellar population. Moving outward from the core, the galaxy displays a subtle gradient in color, transitioning to a slightly bluer tint in the outer regions. This could be attributed to the presence of younger stars or ongoing star formation in the galactic disk. The galaxy appears relatively undisturbed, lacking any pronounced tidal features or signs of recent major mergers. There may be minor disturbances visible in the outer disk. The overall shape is somewhat elongated, suggesting it is not a perfectly spherical elliptical but slightly cigar shaped.
