The galaxy appears as a moderately luminous, elliptical-shaped object, elongated along its major axis. The light distribution suggests a relatively smooth, featureless morphology, lacking prominent spiral arms or distinct substructures. A central bulge is discernible, exhibiting a brighter, more concentrated light profile compared to the outer regions. The overall color appears to be yellowish-orange, possibly indicating an older stellar population with a lower rate of ongoing star formation, and little dust obscuration. There may be a slight disturbance in the overall shape suggesting a past, small merger event.
