The galaxy presents as a fairly smooth, elliptical-like structure, with no obvious spiral arms or significant disk features visible in this image. It exhibits a somewhat concentrated central region which fades outward to a more diffuse halo. The galaxy appears largely featureless, suggesting that the majority of its stars are older, and there is minimal ongoing star formation. There appears to be a tidal tail or small dwarf galaxy merger occurring in the lower portion of the image. Based on its color, the galaxy appears to consist of an older stellar population. Overall, the galaxy appears to be a relaxed, evolved system.
