This galaxy exhibits a clear spiral structure. Two distinct spiral arms are visible, tightly wound around a central bulge. The bulge appears prominent and moderately sized. The disk component is not edge-on. The arms display a generally smooth appearance, with only subtle variations in surface brightness along their length. The presence of a bar structure within the galaxy's core is subtle, but may be present. There may be some evidence of disturbances, suggesting possible interactions or recent mergers, although no significant tidal tails or disrupted features are immediately apparent. The colour distribution suggests ongoing star formation.
