The galaxy presents a primarily smooth, elliptical morphology. It exhibits a concentrated, yellowish-orange central region which suggests an older stellar population with less ongoing star formation. The overall shape appears somewhat elongated, deviating slightly from a perfectly circular form. There are some faint indications of possible disturbances or minor features within the galaxy's halo, but these are not pronounced. Based on the color and morphology, this galaxy is likely a relatively massive, evolved system with a suppressed star formation rate.
