The galaxy presents as a spiral type with a notable disk structure. The arms appear well-defined and emanate from a central bulge. The bulge is moderate in size relative to the disk. Two prominent spiral arms are discernible. The winding of the spiral arms appears moderately tight. There's a suggestion of a bar-like structure crossing the central region, although its presence is somewhat subtle. The overall color profile indicates ongoing star formation. There appears to be a slight asymmetry or disturbance in the galactic structure, possibly suggesting a minor interaction or merger in its recent past.
