The galaxy presents as a single, relatively smooth object with a concentrated central bulge. The light distribution appears roughly elliptical. The core is yellowish/gold, potentially indicative of an older stellar population. There may be some subtle structure in the outer regions of the galaxy, but the image resolution makes it difficult to definitively classify. There are no strong indicators of spiral arm structures or tidal tails indicative of recent mergers. The galaxy's overall color is shifted towards the red end of the spectrum. It is likely not undergoing a period of intense star formation. Based on the roundness of the galaxy, it could be considered an elliptical galaxy. There is no evidence to suggest that this galaxy is currently merging with another galaxy.
