The galaxy presents a morphology consistent with an elliptical type, exhibiting a smooth, diffuse light distribution without prominent spiral arms or a distinct bulge. The object displays a generally rounded shape, with a slight deviation from perfect circularity, presenting an in-between appearance. The galaxy's color profile suggests a population dominated by older stars, indicated by the yellowish-red hues. There is no visually compelling indication of active star formation within the galaxy. The overall structure appears relatively undisturbed, though the light distribution hints at possible faint tidal features or minor disturbances, warranting further investigation. There may also be a merger occurring with this galaxy or it may have completed a merger in the past.
