The galaxy presents a somewhat face-on orientation, displaying a prominent central bulge with a bright nucleus. Faint spiral arm structures emanate from the central region, appearing somewhat flocculent and loosely wound. The color profile exhibits a slightly bluer hue in the outer regions of the disk, suggesting ongoing star formation, while the central bulge displays a yellower, potentially older stellar population. The galaxy appears relatively undisturbed, lacking strong evidence of tidal interactions or major mergers, although some minor irregularities in the outer disk cannot be ruled out. There is some indication of a bar-like structure transecting the nucleus. The overall morphology suggests a late-type spiral galaxy with moderate bulge size and activity.
