This galaxy presents as a flattened, disk-like structure, viewed nearly edge-on from our perspective. The central region exhibits a higher concentration of light, appearing as a smooth, bright bulge. The disk component shows a relatively even color distribution, with a blue hue suggesting the presence of a younger stellar population and ongoing star formation. There is no obvious dust lane bisecting the galaxy, but the overall faintness suggests a low mass. No apparent signs of significant tidal disturbances or interactions with neighboring galaxies are observed, suggesting the galaxy is relatively undisturbed. The smooth light distribution and edge-on presentation make a determination of spiral arm structure difficult.
