The galaxy presents as a somewhat elongated structure. A central, brighter region dominates the core, exhibiting a yellowish-white hue. Diffuse, blue-tinged outer regions extend from this core, suggesting the presence of a stellar disk. There is an indication of faint, asymmetrical features or disturbances in the disk, potentially indicating ongoing interactions or past merger events. Overall, the galaxy appears to be an intermediate system between a disk and a spheroid, with evidence of recent or ongoing star formation in the outer regions.
