The galaxy presents a generally elliptical morphology, though with noticeable features suggesting ongoing or past interactions. There is a central bulge that appears relatively smooth and concentrated, exhibiting a yellowish-white hue, which may indicate a population of older stars. Extending outward from the bulge is a fainter disk component, tilted with respect to our line of sight. 

The disk shows a color gradient, with bluer regions interspersed amongst more reddish areas. This suggests regions of active star formation present within the galaxy. These regions are not well-defined and are slightly irregular.

Overall, the galaxy's light distribution appears relatively smooth, with the light intensity decreasing gradually towards the outer edges. A slight distortion, likely due to an ongoing interaction or merger, is observed in the galaxy's shape.
