The galaxy presents an elliptical morphology, exhibiting a smooth, relatively featureless light distribution. The core appears concentrated, suggesting a significant stellar population. The galaxy displays a yellow-orange hue centrally, potentially indicative of an older stellar population with a lower rate of current star formation. There appears to be ongoing gravitational interaction between the galaxy and a secondary structure, which could be a smaller galaxy or a tidal tail. The secondary structure is more red in color, and possibly more dusty. It is in the beginning stages of a merger. The overall structure is fairly compact.
