The galaxy exhibits a morphology consistent with a spiral galaxy, albeit one undergoing significant disturbance, perhaps merging. Evidence of spiral arms are present but ill-defined, with the northern arm appearing brighter and more prominent. These arms exhibit a dusty appearance, hinting at ongoing star formation regions within. The central bulge of the galaxy is relatively bright and prominent, with an elongated shape. Patches of what seem to be active star forming regions are scattered throughout the disk, with the galaxy exhibiting a fairly irregular and disturbed shape.
