The galaxy presents as a relatively smooth, elliptical structure, exhibiting a high degree of central concentration. The core is notably bright, fading gradually into a less luminous halo. The overall color appears to be a somewhat desaturated white-yellow, suggesting a population of older stars. There is no readily apparent disk structure or spiral arm morphology. The galaxy appears to have a slight elongation along one axis, deviating minimally from a perfectly circular form. The object does not show any obvious signs of ongoing mergers or tidal disturbances, such as extended streams or irregular features.
