The galaxy presents as a flattened, elongated structure, displaying characteristics of a spiral galaxy viewed at a high inclination angle. The central bulge exhibits a smooth, concentrated distribution of light, suggesting a relatively older stellar population. The disk component shows a fainter, more diffuse light distribution extending outwards from the bulge. Some subtle, irregular features are visible, potentially indicating the presence of faint spiral arms or dust lanes, though higher resolution imaging would be needed to confirm this. The color gradients suggest a possible variation in stellar populations, with the central bulge appearing redder compared to the bluer outskirts of the disk. The overall morphology suggests the galaxy is undergoing limited star formation. There's a slight asymmetry in the light distribution, potentially hinting at a minor interaction or internal disturbances.
