The galaxy presents as a somewhat diffuse, centrally concentrated object with a discernible elliptical morphology. The core exhibits a yellowish-white hue, suggesting an older stellar population. Moving outwards from the core, the disk appears bluish, likely indicative of more recent star formation. The overall structure suggests a galaxy undergoing relatively quiescent evolution, without prominent spiral arms or significant signs of recent major merger activity. There may be a slight asymmetry or distortion in the outer regions, which could be indicative of a minor interaction or past merger event. 
