The galaxy presents a generally smooth, elliptical morphology. There are no apparent spiral arms or a distinct disk-like structure. The galaxy's light is concentrated towards the center, with a gradual decrease in intensity outwards. The central region appears slightly more yellow-red in color, suggesting an older stellar population. Fainter blue regions may indicate some recent star formation. There are no obvious signs of a major ongoing merger event, though some subtle asymmetry may suggest minor disturbances. The galaxy is generally round, with a hint of elongation.
