The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. There appears to be a slight elongation to the galaxy's overall shape, although it is mostly round. The core region exhibits a bright, concentrated luminosity, indicative of a dense stellar population or possible active galactic nucleus activity. Progressing outwards from the core, the luminosity gradually decreases. There are hints of subtle color gradients, with a possible shift from yellow-white in the center to bluish-white in the outer regions, possibly indicating the presence of younger stellar populations in the outskirts. No distinct spiral arm structures or prominent dust lanes are visible. The galaxy does not show any obvious signs of major disturbances or ongoing mergers based on the smoothness of its structure. It appears to be a relatively undisturbed system.
