The galaxy presents as a spiral type, observed at a significant angle from face-on. The presence of spiral arms is suggested, though they are not sharply defined, appearing somewhat flocculent in nature. The galaxy features a noticeable central bulge that appears moderately prominent and exhibits a yellowish hue, indicative of an older stellar population. The disk component shows a bluer coloration, suggesting ongoing star formation. There is no evidence of a strong bar structure. The overall morphology indicates a system that is generally undisturbed, with no obvious signs of a recent major merger event, although there appears to be some irregular structure within the disk, and possible faint tidal features.
