The galaxy exhibits a prominent, centrally concentrated bulge, surrounded by a fainter, more diffuse disk. The disk appears to be inclined at an angle, giving the galaxy an elongated appearance. Hints of spiral arm structure are discernible, though not sharply defined. Dust lanes are not clearly visible, but there are some dark patches distributed within the disk. The overall color of the galaxy appears relatively blue, particularly in the outer regions of the disk, suggesting ongoing star formation. The central bulge is brighter, and likely more populated with older stars. There is a slight asymmetry in the outer disk, possibly indicating a minor interaction or disturbance in the past.
