This galaxy exhibits an elongated, disk-like structure with a noticeable bulge in the center. The core appears to be composed of older stellar populations, indicated by its yellowish-orange hue. The disk shows a hint of bluer color, suggesting regions of ongoing star formation. The galaxy’s morphology appears slightly disturbed, with subtle irregularities in its shape. There may be evidence of a minor interaction or past merger event that has perturbed the structure. The overall smooth appearance indicates that it does not show any obvious spiral arm structure.
