The galaxy presents as a flattened, elongated structure, likely a disk galaxy viewed at a high inclination angle. The central bulge appears prominent and concentrated, exhibiting a yellowish-white hue, which suggests an older stellar population and a lack of ongoing star formation. The disk component displays a fainter, bluer coloration extending away from the bulge, indicative of younger stars and potential regions of star formation. The dust lanes are subtly present, obscuring some of the light from the disk and contributing to its mottled appearance. No distinct spiral arms are immediately apparent, and the outer edges of the disk fade gradually into the background, without distinct boundaries, which may indicate an aging galaxy. Overall, the galaxy exhibits a smooth, regular morphology without signs of major disturbances or active galactic nuclei features.
