The galaxy appears to be a spiral galaxy, observed at an angle that is neither perfectly face-on nor perfectly edge-on. The central bulge is moderately sized and exhibits a yellowish-white hue, suggesting an older stellar population. The galaxy displays distinct spiral arms, exhibiting a loose winding pattern. Two prominent arms are clearly visible, emanating from the central bulge. A bar-like structure bisects the bulge, appearing to be a strong bar. The disk component shows regions of bluer light, indicating younger stars and possible ongoing star formation. There is no obvious visual indication of a major merger event, though there are some minor disturbances.
