This galaxy appears to be a spiral galaxy observed at an oblique angle, presenting a somewhat elongated, cigar-shaped profile. The central bulge exhibits a yellowish hue, potentially indicating an older stellar population. Fainter spiral arms emanate from the bulge. The arms present a bluer color, suggestive of ongoing star formation within the galaxy's disk. There may be a slight asymmetry or minor distortions in the spiral arm structure, possibly indicating past interaction or minor disturbance with another galaxy.
