The galaxy presents as a spiral type, with a prominent disk structure. Two well-defined spiral arms are visible, exhibiting a moderate winding pattern. The arms appear somewhat fragmented and asymmetrical, with distinct regions of increased luminosity, potentially indicative of active star formation. The central bulge region is relatively small compared to the overall disk size and displays a smooth, indistinct morphology. The galaxy is oriented approximately face-on relative to our line of sight. There is no indication of a prominent bar structure. There appears to be some minor disturbance to the shape of the galaxy, and some interaction with a nearby object cannot be ruled out.
