The galaxy appears as a centrally concentrated object with a smooth, relatively featureless morphology. Its overall color profile suggests a dominant stellar population of older stars, with a yellowish-golden hue. No distinct spiral arm structure or bar is visible. There is a slight elongation in the overall shape, deviating slightly from a perfectly circular profile. Indications of tidal disturbances or major merger events are absent, and there is no apparent presence of a bright, actively star-forming nucleus or distinct dust lanes. The galaxy appears quiescent, likely an elliptical or lenticular type, and potentially a massive system.
