The galaxy presents as a relatively faint, elongated object. Its shape is noticeably flattened, suggesting a disk-like morphology. The orientation appears to be approximately edge-on, with a clear axis of symmetry. While the image resolution limits detailed observation, there is no immediately obvious presence of strong spiral arm structures or a prominent central bulge. There is some evidence of a slight color gradient along the major axis, with bluer hues potentially indicating ongoing star formation in the outer regions. Overall, the galaxy presents the characteristics of a spiral galaxy observed at a significant inclination. There appears to be limited morphological disruption, suggesting it is not undergoing a major merger event.