The galaxy presents as a somewhat elliptical structure. The central region exhibits a bright, concentrated core, suggesting the presence of a substantial population of stars and potentially an active galactic nucleus. The overall color appears bluish-white, indicative of a population of relatively young, hot stars. A faint disk is suspected, oriented at an angle to our line of sight. There is some subtle structuring present, possibly indicative of spiral arms. A slight distortion in the shape might suggest past interactions with another galaxy, although no obvious merger is readily apparent in the image. Overall, the galaxy appears relatively smooth and quiescent.
