The galaxy presents as a spiral type, exhibiting a flattened disk structure. Prominent spiral arms are discernible, though somewhat tightly wound around a central bulge. The bulge appears moderate in size relative to the disk. The galaxy shows a noticeable degree of inclination, with the disk oriented at a significant angle to our line of sight. The central bulge is bright and yellowish. Fainter blue regions are visible within the spiral arms, likely indicative of recent star formation. The overall color of the galaxy suggests a mix of stellar populations, with a relatively old stellar population in the bulge and younger stars populating the arms. The galaxy does not show any obvious signs of a recent major merger or tidal disruption.
