This galaxy appears to be a spiral galaxy, seen at an angle that is more face-on than edge-on. The central bulge is moderately sized and exhibits a yellowish-white hue, suggesting a population of older stars. The spiral arms are well-defined and show a tightly wound morphology. There is a noticeable blue color within the arms, indicating the presence of younger, hotter stars and ongoing star formation. Several spiral arms branch off from the center, with a possible concentration of three to four arms. The overall structure suggests some disturbance or interaction, though not a major merger, as evidenced by slight asymmetries in the arm structure. Faint tidal features are not readily apparent. The galaxy exhibits a range of spiral arm winding, with sections appearing tightly wound and others somewhat more open.
