The galaxy presents as a relatively compact object with an overall elliptical morphology. The central region displays a smooth, diffuse light profile indicative of an older stellar population. A tidal tail extends from the galaxy, suggesting possible past gravitational interactions or mergers. The galaxy appears to be in the late stages of a merger event, with no major disturbances except the tail. The dominant color is a pale blue, implying intermediate age stars are dominant. There is indication of weak star formation.
