The galaxy presents a somewhat amorphous morphology, appearing largely smooth and centrally concentrated. The central region exhibits a distinct yellow-orange hue, suggesting an older stellar population. There's a suggestion of bluer, less concentrated light surrounding the central bulge, possibly indicating regions of recent star formation. Evidence of potential disturbances are present in the overall light distribution, with some asymmetry noticeable, suggesting a possible interaction or recent merger event. The galaxy's shape is more in-between round and elliptical with slight elongation. 
