The galaxy appears to be a spiral type, viewed at a moderate inclination. Two dominant spiral arms extend outwards from a central region. These arms exhibit a somewhat flocculent structure, with a mix of tightly wound segments and more open, loosely defined regions. The central bulge appears relatively small, and the bar feature seems weak if present. Patches of bluer light are visible within the spiral arms, indicative of star formation regions. There is evidence of some ongoing disturbance or interaction, possibly minor, as evidenced by the slightly irregular morphology. The system doesn't show signs of major mergers, but there are possible tidal features suggesting recent gravitational interaction. Overall, this appears to be a spiral galaxy with active star formation and some signs of gravitational influence.
