The galaxy presents as a roughly elliptical structure, exhibiting a smooth morphology. The central region displays a concentrated luminosity, indicating a prominent galactic nucleus. The light profile appears to gradually diminish from the core outward, with no distinct spiral arm structures visible. The galaxy exhibits color variations, with a central yellowish-white hue transitioning to a more bluish tint in the outer regions. A redder patch of emission appears to be present on one side of the galaxy, possibly indicative of an area of enhanced star formation or dust obscuration. A faint, diffuse halo appears to surround the main galactic body. There is an indication of minor gravitational disturbance in the structure of the galaxy. The galaxy does not appear to be undergoing a major merger.
