This galaxy presents as a disk galaxy, viewed at a relatively high inclination. The central bulge is prominent, exhibiting a yellowish hue, suggestive of an older stellar population. The disk surrounding the bulge shows evidence of spiral structure, though the arms appear somewhat flocculent. Two spiral arms seem most prominent and are moderately wound. Within the disk, a bluer component is observed, indicating regions of active star formation. The overall light distribution suggests a moderate-sized bulge relative to the disk. There's no immediately obvious evidence of a major merger, although some slight asymmetry in the outer disk could indicate a minor interaction or tidal disturbance. A weak bar feature could be present in the center.
