The galaxy appears as a centrally concentrated, relatively smooth object. It exhibits a slight elongation, deviating marginally from a perfectly circular morphology, with an approximate diameter of 8 kpc. Color gradients are subtle, with a suggestion of a bluer core transitioning to redder outer regions. There's no strong evidence of spiral arm structure or significant dust lanes. Indications suggest the system exhibits properties of a relatively evolved galaxy, potentially an elliptical or lenticular type. There are no indications of a major merger event; though, there is the possibility for minor disturbance.
