This galaxy exhibits a spiral morphology, with a prominent, relatively bright central bulge. The spiral arms appear somewhat tightly wound and well-defined, suggesting a classification as an intermediate spiral type. The disk component is clearly visible, displaying a generally flattened structure. Subtle color variations are apparent throughout the galaxy, with the central bulge appearing more yellow, potentially indicating an older stellar population, and the spiral arms exhibiting a bluer hue, suggesting more recent star formation. Faint dust lanes are possibly present within the spiral arms, though the image resolution limits detailed assessment. There is no obvious evidence of any major merger events or tidal disturbances, although some minor asymmetry or disturbance cannot be ruled out based on the image alone. The spiral arms appear multi-armed, exhibiting an arm count of at least three arms. It does not possess a strong bar structure, but the presence of a weak bar is not excluded.