The galaxy presents a smooth, elongated morphology, appearing approximately spheroidal. The primary color is yellowish-white, suggesting a population of older stars. There's a subtle blueish halo enveloping the central region, potentially indicative of some ongoing, though limited, star formation activity. The overall structure lacks prominent spiral arms or a well-defined disk, leaning towards an elliptical classification. There are no obvious signs of recent major merger events or significant tidal disturbances, although a minor asymmetry cannot be entirely ruled out at this resolution. The galaxy exhibits a gradual radial decrease in surface brightness.
