The galaxy presents as a relatively smooth, centrally concentrated object. It appears largely elliptical in shape, with a high degree of circularity. A central bulge region is noticeable, characterized by a bright, concentrated glow. The surrounding galactic disk exhibits a more diffuse luminosity with a hint of spiral structure, though these features appear rather faint and tightly wound, indicating a potentially older stellar population. The overall color of the galaxy is predominantly yellowish-white, suggestive of evolved stars. There is a subtle bluer tinge near the outer regions which could indicate the presence of some younger stars or regions of more active star formation, though the rate seems to be low. There is no evidence of a major ongoing merger, but a small disturbance to the disk on one side is apparent.