This galaxy exhibits a disturbed morphology, indicative of a possible ongoing or recent merger event. The central region shows a complex structure with a bright core, possibly containing an active galactic nucleus or a concentrated star-forming region. Diffuse arms extend outwards with a loosely wound structure, and are likely influenced by gravitational interactions. The presence of several bright knots along the spiral arms suggests ongoing star formation. Overall, the galaxy does not present a well-defined disk structure, suggesting it has a prominent bulge and a relatively late-type spiral classification. 
