The galaxy presents a somewhat irregular morphology, appearing neither purely elliptical nor a well-defined spiral. A central, bright, concentrated region is apparent, possibly indicative of a galactic bulge. The galaxy exhibits a flattened disk-like structure, although not sharply defined. The color distribution suggests variations in stellar populations. The central region is more yellow/orange, potentially indicating an older stellar population. Fainter, bluer regions are present in the outer parts, suggesting ongoing star formation. There is evidence of some disturbance in the disk, hinting at a possible past or ongoing interaction/merger event with another galaxy. A less concentrated, smaller, diffuse object is present close to the galaxy, possibly a dwarf galaxy in the process of merging with the main galaxy. Overall, it looks to be a massive galaxy with moderate star formation.
