The galaxy presents as a highly inclined, likely edge-on, spiral or lenticular system. A prominent bulge is observed, with a roughly rounded appearance. The disk is thin and elongated, exhibiting a relatively smooth texture with no immediately discernible spiral arm structures or distinct dust lanes. The overall morphology is consistent with a well-formed galactic disk with a lack of significant ongoing merger activity or major disturbances. The galaxy is approximately 3.4 arcseconds across at half of its maximum brightness. 
