The galaxy presents an overall elliptical morphology with a slight elongation. The core exhibits a bright, concentrated luminosity profile, suggesting a high stellar density within the galactic nucleus. The inner regions display a yellowish-white color, possibly indicative of an older stellar population. 

Moving outward from the core, there is a gradual decrease in luminosity. A faint, diffuse disk-like structure with some arm structures surrounds the core region, with the disk appearing inclined to our line of sight. The outer regions of the disk show patchy areas that are blueish in color. This suggests some active star forming regions in the galaxy. There is no clear indication of a major ongoing merger, though minor disturbances in the disk's symmetry are visible.
