The galaxy presents as a roughly elliptical, disk-like structure. The central region exhibits a high surface brightness, appearing concentrated and yellowish in color, suggesting an older stellar population. Proceeding outwards from the core, a more diffuse and bluish component is observed within the disk. A slight warp is visible. The morphology suggests a system that is not currently undergoing a major merger. Faint disturbances may be present, but not immediately conclusive. There is no evident spiral structure.
