The galaxy appears to be a lenticular or edge-on spiral galaxy. It exhibits a flattened, elongated shape, indicative of a disk structure viewed at a high inclination angle. There's a discernible central bulge, which is brighter and more concentrated than the outer regions of the disk. The galaxy lacks prominent spiral arms. Overall, the galaxy has a relatively smooth appearance, with a noticeable redder hue, particularly near the center, suggesting a population of older stars. There may be minor distortions visible within the galactic disc. No significant tidal features or signs of recent major mergers are apparent.