The galaxy presents as a relatively compact object. Morphologically, it appears largely smooth in structure, with little evidence of spiral arms or a pronounced disk. It is generally elliptical or spheroid in shape, displaying a moderate degree of roundness, though some elongation or distortion is present. There does not appear to be a major ongoing merger event, nor significant tidal disturbances, although there is potential for minor disruption to the overall structure of the galaxy. The galaxy emits strongly in the blue and green wavelengths.
