The galaxy presents a largely smooth, elliptical morphology. The light is concentrated towards the center, indicating a significant bulge component. The color gradient suggests the presence of older stellar populations, appearing redder in the central regions. There is no clear evidence of spiral arms or a prominent disk. Slight irregularities in the outer regions could indicate minor tidal disturbances or interactions, though the galaxy generally appears relaxed. Based on color, minimal star formation seems to be happening within this galaxy. It's observed at a redshift, indicating it is a distant object.
