This galaxy presents as a spiral type, exhibiting a flattened disk structure. The spiral arms are prominent and well-defined, displaying a winding pattern that transitions from tightly wound near the central bulge to more loosely wound at the periphery. Two distinct spiral arms can be easily discerned, each characterized by a bluish hue suggesting active star formation regions. The central bulge appears relatively small but significant, with a yellowish to reddish tint, potentially indicative of an older stellar population. The overall color profile suggests ongoing star formation within the disk, while the core maintains characteristics of a more mature system. There are no strong signs of major mergers or significant tidal disturbances, with possible minor asymmetric disturbances. A bar structure is not obvious, but there may be a slight central elongation that could be related to a weak bar.
