This galaxy presents as a disk galaxy, viewed nearly edge-on. The central bulge appears prominent and smoothly rounded. A distinct dust lane bisects the disk, obscuring the light from stars behind it, providing evidence of significant interstellar medium content. The color profile suggests a range of stellar populations, with bluer hues potentially indicating younger, star-forming regions, and redder colors likely indicating older populations. There is no obvious evidence of interaction with any nearby galaxies, or any major disruption of the galaxy's overall structure. There is a clear disk but the galaxy otherwise appears to be of relatively undisturbed morphology.
