This galaxy presents as a flattened, disk-shaped system, likely viewed at a high inclination angle from our line of sight. The central region exhibits a brighter, more concentrated luminosity profile, suggesting the presence of a bulge component. The disk component appears relatively smooth, with little evidence of distinct spiral arm structure or intense star formation regions. The color gradient transitions from a yellowish hue in the central bulge to a slightly bluer tone towards the outer edges of the disk, implying a younger stellar population in the periphery. The overall symmetry of the disk is slightly disturbed, indicating potential minor gravitational interactions or internal asymmetries. There is no obvious indication of a recent major merger event. Overall, this galaxy appears to be an intermediate-mass spiral galaxy with a moderate level of ongoing star formation and a stable morphology.
