The galaxy presents a largely smooth, elliptical morphology. It appears highly rounded, exhibiting minimal disk-like features or significant disturbances. The light distribution suggests a relatively homogenous stellar population. The galaxy exhibits a color gradient, shifting from bluer hues in the central region to redder tones toward the outer edges, this may be due to the presence of older stars in the outer regions. The general color suggests moderate ongoing star formation, but not at an exceptional rate. There is no visual evidence of active galactic nucleus activity or a recent major merger event; the galaxy appears to be in a relatively quiescent state.
