The galaxy presents as an elliptical morphology with a smooth, diffuse light distribution. It exhibits a concentrated central bulge, characterized by a yellowish-orange hue, suggesting an older stellar population. The outer regions display a bluer tint, possibly indicating the presence of a younger stellar population or residual star formation within the disk. There's minimal evidence of spiral arm structure or significant dust lanes. The overall appearance suggests a mature galaxy undergoing limited ongoing star formation. There is a slight distortion, possibly a minor disturbance.
