The observed galaxy presents a moderately inclined disk morphology. There is a bright central bulge that appears smooth and slightly elongated perpendicular to the disk, with an intense concentration of light in the galactic nucleus. The disk exhibits a clear color gradient, showing redder hues along its edges and transitioning to bluer tones closer to the central bulge. While the overall structure appears relatively undisturbed, subtle irregularities in the disk's light distribution suggest the possible presence of minor disturbances. The galaxy lacks any readily discernible spiral arm structure within the limits of image resolution.
