The galaxy presents as a disk galaxy with a prominent, though not dominant, spiral structure. There appears to be some disruption in its morphology suggesting a possible interaction or merger event. The spiral arms exhibit a patchy structure, interspersed with bright, blue knots indicating regions of active star formation. The central region is somewhat diffuse, showing a faint concentration of light but lacking a clearly defined bulge. The galaxy is neither perfectly face-on nor edge-on. It exhibits a slight inclination, allowing some glimpse into its disk structure. Evidence of a stellar bar structure is not immediately apparent. The galaxy appears to be undergoing a period of active star formation, distributed throughout its spiral arms. There is a noticeable asymmetry to the distribution of starlight, with one side of the galaxy appearing more disturbed or disrupted than the other.
