The object presents as a single, relatively compact galaxy. It exhibits a smooth, elliptical morphology, with no discernible spiral arms or bar structures. The galaxy's light profile appears concentrated towards the center, suggesting a prominent bulge component. There is a slight color gradient, with the central region exhibiting a more reddish hue compared to the outer regions, which appear slightly bluer. This may indicate older stellar populations dominating the core, with some ongoing or recent star formation in the outer parts. There are no apparent signs of tidal disturbances or close companions, suggesting it is not currently undergoing a major merger, though it is likely to have merged previously with a smaller galaxy. There is a lack of any obvious dust lanes or prominent star-forming regions. The overall appearance suggests that this galaxy is likely a mature system, possibly transitioning toward a more quiescent state.
