The galaxy presents an elliptical morphology, exhibiting a relatively smooth, diffuse structure. A central bulge appears prominent, with a concentration of light suggesting an older stellar population. The overall color gradient transitions from a yellowish core to slightly redder hues in the outer regions, indicating potential variations in stellar age and metallicity. There is a slight asymmetry to the galaxy's shape, but it otherwise appears undisturbed. Based on the color and texture, the galaxy exhibits low rates of star formation.