The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The light profile appears brightest towards the core, gradually diminishing in intensity outwards. A slight elongation is observed; however, there is no evident spiral arm structure. A slight colour gradient is seen, with a redder core transitioning to slightly bluer hues in the outer regions. The overall color suggests an older stellar population. No significant dust lanes or regions of active star formation are immediately apparent within this image. A high likelihood of non-disturbed morphology.
