The galaxy appears as a single, somewhat smooth structure with moderate levels of star formation. The galaxy exhibits an elliptical morphology, with the light profile appearing to be concentrated at the center. The galaxy exhibits a color gradient. There is a higher concentration of green light towards the core of the object and a higher concentration of red and blue light towards the outer edges of the object. There is evidence of some tidal activity, potentially suggesting an ongoing or past merger event. These tidal forces may be the result of a galaxy merger. There is no evidence of a distinct disk structure, but a smooth central bulge is visible.
