The galaxy appears to be an elliptical type, exhibiting a generally smooth, featureless morphology with a concentrated central bulge. It has an elongated shape, deviating significantly from being perfectly circular. The color gradient transitions from a bright, yellowish-orange core to a more subdued greenish-blue outer region. There are no apparent spiral arms or distinct dust lanes visible. The overall structure suggests the possibility of a relatively evolved system with a dominant older stellar population. However, subtle color variations could also indicate ongoing, though possibly limited, star formation activity in certain regions. There may be a minor gravitational disturbance present.
