The galaxy presents as an elliptical structure with a smooth, diffuse light distribution. There is a noticeable color gradient, with the central region appearing more yellow/white, suggesting an older stellar population and lower star formation rates. The outer regions are slightly bluer, potentially indicating the presence of some younger stars, though this is less pronounced. The galaxy exhibits a cigar shape. There is no clear evidence of spiral arm structure or a prominent dust lane. Overall, the morphology indicates a relatively evolved galaxy with a dominant spheroid component.
