This galaxy appears to be a spiral galaxy, viewed edge-on from our line of sight. It exhibits a distinct disk structure, with a bright, central bulge region. The bulge appears somewhat rounded. There is evidence of dust lanes within the disk, appearing as subtle dark patches silhouetted against the light of the stars. The galaxy's color suggests the presence of both young, blue stars and older, redder stellar populations. A noticeable warp is either present in the galaxy, or it is undergoing some kind of disturbance from a neighbor. There also seems to be a high star formation rate within this galaxy.