The galaxy presents a distinct spiral morphology, appearing nearly edge-on from our vantage point. Two prominent spiral arms can be discerned, loosely wound around the central bulge. The arms exhibit a patchy distribution of star formation, indicated by regions of blue light, potentially marking areas of active star birth. A noticeable dust lane bisects the galaxy, obscuring a clear view of the galactic center. The central bulge appears moderately sized with a yellowish hue, possibly indicative of an older stellar population. There is some distortion in the symmetry of the disk, potentially indicating ongoing or past interactions with another galaxy.
