The galaxy presents as a somewhat face-on spiral galaxy with an apparent smooth morphology. A central bulge with a yellow-orange hue dominates the galactic structure, indicative of an older stellar population. Fainter spiral arms are observed extending outwards from the bulge, displaying a bluer tint, suggestive of more recent star formation activity. The galaxy's disk appears relatively undisturbed, showing no signs of major merger events, although there might be minor disturbances in the outer regions. Overall, the galaxy exhibits a moderate level of star formation.
