The galaxy presents as a spiral system with a prominent central bulge. The bulge appears smooth and concentrated, with decreasing luminosity moving outwards. A disk is evident, displaying spiral arm structure. These arms are tightly wound, creating a complex and somewhat flocculent appearance. The orientation of the galaxy to the line of sight is somewhere between face-on and edge-on. The bluer colors hint at the likelihood of ongoing star formation regions within the disk, particularly along the spiral arms. A weak bar may be present in the central region. The galaxy exhibits overall fairly symmetrical morphology. There is no visual evidence of a major merger or significant tidal disturbance.
