The galaxy presents a relatively smooth, rounded morphology, indicative of an elliptical or S0-type galaxy. There is no discernible spiral arm structure. The central region exhibits a high degree of concentration of light, suggesting a prominent bulge. The color appears yellowish-red, possibly indicating an older stellar population and a relatively low rate of on-going star formation. There is no obvious evidence of tidal tails or strong interactions with other galaxies, although a faint, diffuse halo might be present. The overall appearance suggests a well-evolved system with a significant stellar mass. Some irregularities in light distribution suggest the possibility of minor disturbances.