The galaxy presents as a relatively bright, face-on spiral galaxy. A prominent central bulge dominates the core, exhibiting a yellowish hue, suggestive of an older stellar population. Fainter spiral arms extend outwards from the central region, showing hints of blue, which may indicate ongoing star formation. The disk appears somewhat flocculent. There is some suggestion of interaction with other objects, or internal disturbance, but overall the disk is not heavily disrupted. There is no noticeable bar structure. The galaxy's overall form indicates that it is in a relatively late stage of its evolution, likely containing a mix of stellar populations and ongoing star formation within its spiral arms.
