The galaxy appears to be a relatively smooth, elliptical-like structure with a concentrated central bulge. It exhibits a yellowish-red hue, suggesting an older stellar population with fewer young, massive stars. There's a noticeable lack of distinct spiral arms or prominent dust lanes, which further supports the classification of an early-type galaxy. The galaxy's morphology is generally regular, without obvious signs of major tidal disturbances or ongoing mergers, though there may be some minor asymmetry present. Overall, the galaxy seems to be a mature system.
