The galaxy presents as a spiral type, oriented approximately face-on to our line of sight. A prominent central bulge is evident, exhibiting a yellowish hue suggestive of an older stellar population. Loosely defined spiral arms extend outwards from the bulge. The arms show some patchiness with regions that appear bluer, likely indicating active star formation. The overall structure shows some degree of disruption, with the arm structure not fully symmetrical which may be the result of a minor disturbance. There is no evident bar feature in the galactic center. The disk shows moderate prominence compared to the bulge. No major merger event is ongoing.
