The galaxy appears as a relatively smooth, elliptical-like structure with a slightly elongated shape. There is a brighter, more concentrated central region suggestive of a bulge. The outer regions of the galaxy show a gradual decrease in surface brightness, fading into the background sky. The color is predominantly bluish, hinting at a population of younger, hotter stars, possibly indicating ongoing star formation. There is a subtle suggestion of a disk-like component, though the overall smoothness dominates the morphology. There does not appear to be any strong tidal features, indicating that it is not currently undergoing a major merger, although there is the possibility of some minor disturbances.
