The galaxy presents a clear, elongated morphology. The primary axis is significantly longer than its minor axis, indicating a highly flattened, disk-like structure viewed nearly edge-on. The central region exhibits a high degree of luminosity, appearing bright and concentrated. The color gradient transitions smoothly from a yellowish-white core, suggesting an older stellar population, to fainter bluish hues at the outer edges of the disk, which is potentially indicative of ongoing star formation. There are no apparent signs of major mergers or significant tidal disturbances. Overall, the galaxy appears to be a relatively undisturbed disk galaxy with intermediate mass and moderate star formation.
