The galaxy appears as an elliptical or lenticular type, exhibiting a smooth, relatively featureless morphology. The light distribution suggests a centrally concentrated spheroid of stars. The galaxy displays a yellowish-orange hue in the central region, potentially indicative of an older stellar population. A slight elongation is visible, hinting at a possible disklike structure viewed at an angle, but this is not distinct. There are no noticeable spiral arms, dust lanes, or regions of active star formation readily apparent. The smooth appearance and lack of significant morphological disturbances suggest the galaxy is likely a relatively settled system that has not experienced a major merger event recently.
