The galaxy appears to be a disk galaxy, observed at an oblique angle. The central bulge is pronounced and exhibits a yellowish hue, suggesting an older stellar population and a low rate of current star formation in that region. The disk itself is subtly visible, appearing somewhat flattened and extending beyond the central bulge. Faint, bluer regions can be discerned within the disk, potentially indicating areas of ongoing star formation. The spiral arms, if present, are not sharply defined in the available image. There is no obvious evidence of a major merger, tidal tails, or significant morphological disturbances, though a minor asymmetry cannot be ruled out. The galaxy exhibits a moderate degree of smoothness.
