The galaxy presents as a relatively face-on spiral with a distinct central bulge. The spiral arms appear somewhat flocculent and not tightly wound. Star formation appears moderate within the arms, with a possible hint of HII regions. There is some asymmetry to the spiral structure, indicating possible minor gravitational interaction or recent merger event. Dust lanes are visible within the arms, particularly on the left. The central bulge is bright and shows a smooth light distribution, likely populated by an older stellar population. The disk of the galaxy appears to extend moderately with an approximate diameter of about 6 kpc. The galaxy exhibits a slightly bluish tint in the disk, indicating the presence of younger stars.
