The galaxy presents as a spiral type, exhibiting a clear disk structure. Two prominent spiral arms can be discerned. The spiral arms are moderately wound. A central bulge is readily apparent, appearing to occupy a significant portion of the galaxy's overall structure. The bulge appears to be of moderate size relative to the disk. The galactic disk appears slightly inclined relative to the observer's line of sight. There is no evidence of a major ongoing merger. The galaxy's features are suggestive of moderate ongoing star formation. 
