The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. The core exhibits a yellowish-white hue, indicative of an older stellar population. The isophotes appear largely regular, transitioning to a fainter, less defined halo or envelope. The galaxy displays a slight ellipticity, deviating somewhat from a perfectly circular form. There is no obvious evidence of spiral arms or significant dust lanes. The overall appearance suggests an evolved system, possibly an elliptical or lenticular galaxy, with a relatively low rate of ongoing star formation. There appear to be no signs of any major merger events or tidal disturbances.
