The galaxy presents a flattened, elliptical morphology. A bright, concentrated central bulge dominates the overall luminosity. The bulge exhibits a smooth, relatively featureless appearance. A faint, diffuse disk surrounds the central bulge, displaying a slightly bluer color than the bulge. No distinct spiral arm structure is discernible within the disk. The outer regions of the galaxy gradually fade into the background sky, indicating a decreasing stellar density. The galaxy does not exhibit any obvious signs of ongoing major merger activity, but some minor disturbance within the disk cannot be ruled out based on this image alone. The overall color suggests a relatively evolved stellar population. The estimated size indicates it is a moderately sized galaxy.
