This galaxy presents a largely smooth, elliptical morphology. The central bulge exhibits a concentrated, yellowish hue, suggesting a population of older, redder stars. A faint, diffuse disk is visible, extending outwards from the bulge. This outer region displays a bluer color, indicative of some ongoing, though perhaps relatively low-level, star formation. There are no readily apparent signs of significant disturbances such as tidal tails or asymmetries that would suggest a recent major merger. The overall round shape implies minimal angular momentum. The galaxy's color gradient suggests a decrease in the average stellar age with increasing distance from the galactic center.
