The galaxy presents as a disk-shaped system, exhibiting a generally blue hue, suggestive of active star formation. Its morphology appears disturbed, with a noticeable asymmetry. A bright central bulge is visible, yet appears to be disrupted from a relaxed state. Distinct clumps or knots of brighter blue light are present within the disk, perhaps indicative of massive star clusters or HII regions. The overall structure lacks a well-defined spiral arm pattern; the disk appears patchy and irregular. It is possible the system is interacting with another, or that it has undergone a recent merger, evidenced by the disturbed morphology and starburst activity. A slight dust lane may be present but is not clearly defined. The visible extent of the galaxy is relatively compact.
