The galaxy appears to be a relatively smooth and centrally concentrated system, exhibiting an elliptical morphology. The light distribution is diffuse, showing a gradual decline in brightness from the core outwards. The galaxy is not perfectly spherical, displaying a slight elongation along one axis, it seems to be more rounded than cigar shaped. There is no evidence of spiral arm structure or prominent dust lanes. There is a slight distortion to its structure, and it is likely that it is a minor disturbance but not currently in a merging phase. The primary color of the galaxy is whitish-yellow, suggesting an older stellar population with less ongoing star formation. No distinct regions of star formation are visible.
