The galaxy appears to be an elliptical galaxy, characterized by a generally smooth and featureless morphology. It presents a concentrated central bulge that emits primarily in yellow and red wavelengths, suggesting an older stellar population. The outskirts of the galaxy exhibit a gradual decrease in surface brightness, fading into the background sky. There is little evidence of spiral arms, dust lanes, or ongoing star formation. The overall shape is mostly round, lacking any significant distortions or tidal features indicating recent interactions. The galaxy appears isolated, with no other objects noticeably disturbing its structure.
