This galaxy exhibits a generally smooth morphology, with a high degree of central concentration and a relatively round shape. It presents a bright, yellowish core which gradually fades into a bluer, diffuse outer region. There's some indication of very subtle, ill-defined spiral arms, but they are poorly formed and mostly indistinct. Overall, it appears to be a massive galaxy, with an estimated median star formation rate that is quite low. We detect no significant mergers or tidal disturbances, suggesting that it is a relatively undisturbed galaxy. The observed colors suggest an older stellar population with a low dust content.
