The galaxy presents a flattened, disk-like morphology, observed at a significant inclination. Its central region exhibits a concentrated luminosity, appearing yellowish-white, indicating a likely older stellar population dominating the core. Fainter, more diffuse light extends from the core along the major axis, transitioning towards a slightly bluer hue at the outer edges of the disk. This suggests some ongoing star formation is present in the disk, albeit at a lower rate. Overall, the galaxy's structure appears relatively undisturbed, showing no signs of major mergers or significant tidal features. The primary structure is smooth, but some irregularity is observed in the disk, suggesting some minor disturbances or internal processes.
