The galaxy in the image presents a predominantly smooth morphology. Its overall shape appears close to round. There is no apparent evidence of a significant disk component or spiral arm structures. Faint irregularities suggest possible minor disturbances. The galaxy exhibits a yellowish color, potentially indicating an older stellar population with reduced ongoing star formation. The estimated size indicates it is a sizable galaxy. The central region appears slightly brighter, possibly indicating a higher concentration of stars or the presence of an active galactic nucleus. The galaxy appears relatively isolated, with no immediately apparent signs of major ongoing merger activity, although faint disturbances cannot be ruled out.
