This galaxy appears to be a spiral type, viewed at an angle between face-on and inclined. Two spiral arms emanate from the central bulge, which is slightly elongated. The arms are not tightly wound, displaying a somewhat open morphology. Star formation appears to be actively occurring within the spiral arms, as evidenced by the presence of several bright regions. The central bulge exhibits a yellowish-orange hue, suggesting an older stellar population. The overall structure shows some signs of minor gravitational disturbance, although the main galactic structure is well maintained. There does not seem to be a strong central bar.
