The galaxy presents as a somewhat disturbed spiral. There is a central bulge which appears bright and yellowish-white. Extending outwards from the bulge, there is evidence of a disk. The disk appears diffuse with faint spiral arms visible. One side of the disk has an irregular shape, suggesting a possible interaction or tidal disturbance. The overall color of the disk is slightly bluer than the bulge, indicating younger stellar populations, particularly in regions of active star formation. The galaxy is not a pure elliptical, though it may be categorized as a late-type spiral experiencing some degree of disruption.
