The galaxy presents as a lenticular or edge-on spiral type, exhibiting a flattened, elongated morphology. Its core appears bright and concentrated, suggesting a substantial bulge component. The disk is discernible, though lacking in high-resolution details, and displays a smooth, featureless texture, lacking prominent spiral arm structures or distinct dust lanes. The color profile indicates a yellow-white hue, suggesting a population dominated by older stars, with relatively suppressed ongoing star formation. The overall structure indicates a relatively evolved galaxy, possibly undergoing a transition from spiral to elliptical morphology, or a disk galaxy viewed at a high inclination angle. There is little to no evidence of active galactic nucleus activity or recent mergers in this image. 
