The galaxy presents as a centrally concentrated system, elongated in shape, with a discernible bulge. The color profile suggests an older stellar population dominates, particularly within the central region, exhibiting a yellowish-red hue. Fainter blue extensions suggest the presence of a disk, although poorly resolved. The galaxy appears relatively smooth, with little indication of prominent spiral arms or significant dust lanes. The overall morphology implies it is likely an elliptical or lenticular galaxy. It is likely a relatively massive galaxy with ongoing but not extreme star formation. There is some slight evidence of a tidal disturbance, perhaps an early stage merger.
