The galaxy presents as a relatively smooth, elongated structure. The central bulge exhibits a concentrated luminosity, appearing nearly spheroidal and possessing a slightly reddish hue. Moving outward from the core, a more diffuse disk is observed. This disk shows a bluer coloration, with a slight flattening. The shape suggests a possible classification as an elliptical galaxy. There appears to be minimal evidence of ongoing major mergers, or significant tidal disturbances, although a very slight asymmetry cannot be ruled out without further investigation. The overall light profile appears to lack prominent spiral arm structures or dust lanes, reinforcing the smooth morphological characteristic.
