The galaxy appears to be an elliptical galaxy, characterized by a smooth, featureless light distribution. The galaxy's shape is generally round, with a slight deviation from perfect circularity. No distinct spiral arms or bar structures are visible. The central region of the galaxy exhibits a high concentration of light, gradually decreasing towards the outer edges. The overall color of the galaxy suggests an older stellar population, with a reddish-yellow hue. There is no evidence of major disturbances or ongoing mergers, although a minor asymmetry cannot be ruled out. The galaxy's estimated size is a few kiloparsecs across. Based on the overall appearance, this galaxy is consistent with a relatively massive system, possessing a substantial stellar mass.
