The galaxy presents as a spiral type, with two prominent spiral arms easily discernible. These arms exhibit a flocculent structure, appearing somewhat patchy and less well-defined. The winding of the spiral arms appears to be a medium tightness, that is, neither tightly wound nor loosely extending. The galaxy possesses a noticeable bulge, of moderate size, and appears to be a barred spiral galaxy with a weak bar structure. The disk exhibits a slight inclination. There is evidence of a minor disturbance within the galaxy, but no signs of a major merger event. Star formation is ongoing, with blue light indicating the presence of young, hot stars in the spiral arms.
