The galaxy presents as a relatively smooth, disk-like structure viewed at an intermediate angle, appearing somewhat elongated but not strongly cigar-shaped. The central bulge exhibits a yellowish hue, suggesting an older stellar population. Fainter, bluer regions are interspersed within the disk, possibly indicating ongoing star formation. There is a hint of some disturbance in the disk, possibly some early stages of a minor disturbance event, but the overall structure remains largely intact. It is likely a fairly massive galaxy.
