The galaxy presents a flattened, elliptical morphology, exhibiting a smooth and diffuse light distribution. The central region appears bright and concentrated, indicative of a prominent bulge. Moving outwards from the core, the light gradually fades into a fainter, less defined halo. The galaxy is not perfectly symmetrical but shows only minor disturbances. Overall, the galaxy appears to be a relatively undisturbed system with no major signs of recent merging activity.
