The galaxy presents a somewhat irregular morphology, suggestive of a spiral structure. Faint spiral arms are visible, though not sharply defined. The arms appear to wind loosely around a central region. There is evidence of substantial star formation occurring within the arms, indicated by the patchy, bluer concentrations of light. The galaxy does not appear to be perfectly smooth, and exhibits minor disturbances, possibly indications of tidal interactions or recent accretion events. There is not a well-defined central bulge, the galaxy appears more disk dominated. A weak bar structure is potentially present, as the core area is elongated. Overall, the galaxy appears to be in a dynamically active state, showcasing ongoing star formation and a slightly disturbed morphology.
