The galaxy presents as a centrally concentrated object, exhibiting a smooth, slightly elongated morphology. The color profile appears relatively uniform across the galaxy, tending toward warmer hues, predominantly orange, which suggests an older stellar population and possible ongoing, moderate star formation. There is a subtle suggestion of a disk-like structure, though the smoothness of the light distribution implies it is not highly defined or actively star-forming across its entirety. There is a minor disturbance, possibly indicative of a small interaction or past merger event. Overall, the galaxy presents a transitional appearance between a spiral and elliptical galaxy.
