The galaxy presents as a spiral type, observed at an angle approaching edge-on but with some disk visibility. The central bulge appears prominent and possesses a yellow-white hue, suggestive of an older stellar population.

Spiral arms are present, with some showing tighter winding. The disk is bluish, possibly indicating ongoing star formation within the spiral arms. Some areas of the spiral arms seem somewhat clumpy, which may represent regions of increased star formation. There is no obvious indication of a strong bar structure. The morphology doesn't suggest a recent major merger event, but some minor disturbances in the disk's symmetry cannot be ruled out.
