The galaxy presents a prominent disk-like structure. The disk exhibits a clear spiral pattern. The spiral arms appear relatively tightly wound. A central bulge is observable, with an intermediate prominence. The light distribution suggests moderate star formation activity, with some blue light emanating from the spiral arms, but the galaxy does show a strong yellowing which may suggest it has a lower rate of star formation. The galaxy shows some evidence of a bar structure, with a slightly elongated central region, or two regions of high light concentration on either side of the central core. There is no evidence of major tidal disturbances or ongoing major merger activity.
