The galaxy presents as a relatively smooth, disk-like structure with a prominent central bulge. The bulge exhibits a concentrated yellowish hue, suggesting an older stellar population. Extending outwards from the bulge, a fainter, greenish disk is observed. The disk appears relatively undisturbed, lacking strong evidence of spiral arm structure or significant dust lanes. There might be the slightest hint of a very small spiral structure but I can't confirm from this image. The overall shape of the galaxy is more rounded than elongated, though with the hint of a slight cigar shape. The galaxy's general smoothness and lack of major disturbances indicate it is likely a relatively evolved system and not actively undergoing a major merger event.
