The galaxy presents as a relatively face-on spiral, exhibiting a moderate bulge component. The spiral arms are somewhat flocculent in nature and are traced by regions of bluer light, suggestive of ongoing star formation. There appears to be no strong bar structure. The overall color is intermediate, with some degree of dust attenuation possibly present. There may be some minor interaction or disturbance in the outskirts of the galaxy. The estimated size indicates a moderate scale, with significant HI presence.
