The galaxy appears as a relatively smooth, elliptical-shaped object. The central region exhibits a bright, concentrated luminosity, suggesting a substantial stellar population and/or active galactic nucleus. The light intensity gradually decreases from the core outwards.

There is a subtle color gradient observed, with the central region appearing more yellow, and the outer edges possessing a slightly bluer hue. This may indicate differences in stellar populations, with older, redder stars concentrated in the core and younger, bluer stars in the outskirts.

There is no obvious spiral structure or significant dust lane visible in the image, lending support to the galaxy's classification as elliptical. There is no major disturbance or merger apparent. It appears fairly isolated in its immediate surroundings.