The galaxy appears as a diffuse, centrally concentrated object with a relatively smooth morphology. There is a subtle elongation, suggesting a shape that deviates slightly from perfect circularity. The core exhibits a brighter, yellowish-white hue, possibly indicating an older stellar population and/or dust obscuration. Fainter, less distinct disk-like structures or extensions are faintly visible, hinting at a spiral or lenticular galaxy type. There's a hint of bluer regions, possibly indicating some star formation, but overall the galaxy seems to be dominated by older stars. Based on the morphology, it is likely a galaxy undergoing or having completed a transition from a more active, star-forming state to a more quiescent phase. Possible minor disturbance in the galaxy shape shows evidence of the possibility of merger activity. 
