The galaxy presents as a spiral type, observed at an oblique angle, though not quite edge-on. A distinct bulge, seemingly of moderate size, is visible at the galaxy's core. The bulge exhibits a yellowish hue, potentially indicating an older stellar population. The disk shows evidence of spiral arm structure, although the arms appear somewhat patchy and not sharply defined. Bluer regions within the disk are suggestive of ongoing star formation. A bar structure appears to be present, extending from the central bulge. There is no obvious visual indication of a major merger event, although there might be some subtle distortion in the outer disk which could be indicative of a minor disturbance. Overall, the galaxy appears relatively undisturbed.
