The galaxy presents a largely smooth and centrally concentrated morphology. It exhibits a prominent, bright central bulge transitioning into a more diffuse and slightly elongated halo. The color profile suggests an older stellar population, with a yellowish-red hue dominating the central regions. There is little evidence of spiral arm structure or significant dust lanes. Minor asymmetrical light distribution might imply slight tidal disturbances or a minor recent interaction, although it is difficult to ascertain definitively with the available image resolution. The overall structure implies this is likely an elliptical galaxy.