The galaxy presents as a face-on spiral galaxy with a prominent central bulge. The bulge exhibits a yellowish-white hue, indicative of an older stellar population. Fainter, bluish spiral arms extend outwards from the central bulge. These arms are somewhat flocculent in nature, with patchy regions of star formation visible as bluer knots embedded within the arms. The disk component appears relatively smooth, with moderate dust lanes that are slightly apparent within the spiral arm structures. The overall shape appears slightly elongated, suggesting a possible weak bar structure or asymmetry in the distribution of the stellar mass.
