The galaxy presents an elliptical morphology, exhibiting a smooth light distribution with a high degree of central concentration. The galaxy appears to be dominated by an older stellar population, indicated by the yellowish-orange hue of the central bulge. Fainter, bluer light extends outwards from the central region, suggesting the presence of a younger, star-forming stellar population in the outer regions, but it is not prominent. The isophotes, while slightly elongated, lack significant disturbances, suggesting that the galaxy is not undergoing a major merger event. The overall appearance suggests a relatively quiescent galaxy that has undergone significant evolution.
