The galaxy presents as a relatively smooth, concentrated object. Its morphology suggests a system with a dominant spheroid component, likely an elliptical galaxy or a lenticular galaxy viewed face-on. The galaxy exhibits an overall yellowish hue, indicative of an older stellar population with fewer young, hot stars, and a relatively low ongoing star formation rate. The color gradient appears fairly uniform across the galaxy, with a slightly redder core. There's a possibility of minor disturbances or interactions, based on some asymmetry.
