The galaxy presents a flattened, elliptical morphology, classified as a smooth galaxy. Its overall structure appears relatively undisturbed, showing no signs of major mergers or significant tidal distortions. The central region exhibits a concentrated, bright core, possibly indicative of an older stellar population. Surrounding the core, a more diffuse and less luminous halo extends outwards. There are hints of possible star formation or younger stellar populations within the disk, evidenced by a subtle greenish hue. The overall color profile suggests a mixed stellar population, with older, redder stars concentrated in the bulge and potentially younger, bluer stars scattered within the disk. The galaxy's elongated shape suggests that we are observing it at an oblique angle.
