The galaxy appears as a singular, concentrated object with a generally smooth morphology. There is no apparent spiral structure or distinct disk features visible at this resolution. The central region presents a relatively bright, possibly older stellar population, indicated by its yellowish to reddish hue. It is generally elliptical or spheroidal in shape, with a slight deviation from perfect circularity. There are no obvious signs of recent major mergers or tidal disturbances, though the presence of minor disturbances cannot be ruled out. The galaxy exhibits a considerable luminosity, suggesting it is a massive system. Star formation is likely suppressed.
