The galaxy presents as a somewhat elliptical structure. The central bulge is prominent, exhibiting a high surface brightness and a yellowish-orange hue, suggesting an older stellar population. The galaxy appears relatively smooth in texture, with a fairly high Sersic index, indicating that most of the light is concentrated in the center. There is some flattening visible, but the ellipticity is not extreme. The outer regions of the galaxy are fainter and less well-defined, with a gradual decline in brightness. There is not much in the way of discernible spiral arm structure or dust lanes, and there may be some signs of interaction or disturbance in the outer halo of the galaxy. Overall, the light profile suggests this could be an early-type spiral or elliptical galaxy.