The galaxy presents as a face-on spiral, with a prominent central bulge that transitions into a diffuse disk. The spiral arms are not tightly wound but display an open morphology, with moderate fragmentation and noticeable star-forming regions evident as subtle color variations along the arms. The disk exhibits a mottled appearance, possibly indicating ongoing or recent minor interactions. There is some level of disturbance or asymmetry to the galaxy's overall structure, indicative of recent activity such as minor mergers or tidal interactions, but it is not a highly disrupted system. The color gradients suggest active star formation within the disk, while the bulge shows a characteristic yellow-white hue, suggestive of an older stellar population. The galaxy is likely a moderately massive system with ongoing star formation.
