The galaxy appears to be a relatively smooth, elliptical-like structure. Its core exhibits a bright, concentrated luminosity, suggestive of a significant stellar population or an active galactic nucleus. The surrounding region shows a gradual decrease in light intensity. There is some subtle disc like structure, and potential signs of disturbance. The observed color profile seems to indicate a dominant population of older stars, giving it a yellowish hue, and the estimated size indicates it is a relatively large galaxy. Its characteristics suggest it may be nearing the end of its star-forming phase, or possesses a low star formation rate. The galaxy is likely quite massive.
