The galaxy appears to be an elliptical galaxy, showing a generally smooth, concentrated morphology. It exhibits a yellowish hue, suggesting an older stellar population. There may be little to no ongoing star formation. The galaxy shows an overall round shape, and exhibits no clear signs of disturbances or mergers based on its structural integrity. The estimated size appears to be moderate. The light profile suggests a fairly homogenous distribution of stellar density, with a gradual decrease in intensity from the center outwards, consistent with a relatively evolved system.
