The galaxy exhibits a generally smooth morphology, suggestive of an evolved system. It is elongated in shape, appearing as a flattened disk viewed at a high inclination, nearing edge-on. The central bulge is prominent and exhibits a yellowish hue, potentially indicative of an older stellar population. The disk displays a bluer color gradient toward the outer edges, possibly due to ongoing star formation or a younger stellar population. There may be a slight warp or disturbance in the disk morphology. Overall, the galaxy's structure suggests a spiral or lenticular type, undergoing some form of recent or ongoing evolutionary process.