The galaxy appears to be an elliptical or lenticular type, exhibiting a largely smooth and centrally concentrated light distribution. A slight elongation is observed, deviating from a perfectly circular shape. The core region presents a yellowish hue, indicative of an older stellar population dominating the central bulge. Fainter, bluer regions are present in the outer portions, suggesting the presence of some younger stars and potential ongoing, though likely subdued, star formation activity. There is no apparent spiral arm structure or significant dust lane features visible in this image. The galaxy exhibits minor signs of possible interaction or disturbance in its outer regions. 
