The galaxy appears as a centrally concentrated object with a generally smooth morphology. There's a subtle elongation visible; it's not perfectly spherical but leans more towards a rounded shape. The central region displays a brighter, yellowish-white glow, suggesting an older stellar population. Fainter bluish hues are observed in the outer regions, possibly indicating areas of more recent, albeit suppressed, star formation. There are no prominent spiral arms or a distinct disk. There does not appear to be signs of any major ongoing merging activity, though minor disturbances cannot be ruled out. The overall structure seems relatively undisturbed, indicating a stable, settled system.
