The galaxy presents as a concentrated elliptical form with a smooth, largely featureless appearance. A bright, somewhat diffuse central bulge is clearly visible. Moving outwards from the core, the light gradually decreases without any prominent spiral arm structures, bars, or dust lanes. The shape approximates a rounded form, with only a slight deviation from perfect circularity. Color gradients are subtle; the central regions appear more yellow, possibly indicating an older stellar population, whereas the outer halo exhibits a slightly redder hue. There is no indication of any ongoing major merger events, although there may be a minor disturbance in the morphology. Overall, the galaxy seems like a mature system with a relatively quiescent star formation history.