The galaxy presents as a relatively compact object, roughly elliptical in form. Its central region is noticeably brighter, exhibiting a concentrated core. The overall light distribution appears smooth, suggesting a lack of prominent spiral arms or distinct substructures. There's a slight elongation along one axis, but the galaxy approximates a circular shape. Color gradients are subtle; the core shows a slight shift toward bluer wavelengths, while the outer regions exhibit a redder hue. Faint, diffuse extensions might be present, but the signal-to-noise ratio is low in those areas. Evidence for significant tidal disturbances or major mergers is absent; the system appears relatively undisturbed.
