The galaxy appears to be a disk galaxy, seen nearly edge-on. There is a noticeable central bulge, exhibiting a yellowish-orange hue which could indicate an older stellar population. The disk appears relatively smooth, with only slight indications of substructure. The bluer colors visible along the outer edges of the disk may indicate regions of active star formation. There is no obvious sign of a strong bar structure or spiral arms from this angle. Overall, the galaxy presents a somewhat lenticular-like appearance, but shows signs of ongoing star formation. There are hints of a faint, extended halo surrounding the main body of the galaxy, which may suggest an extensive collection of stars. There does not appear to be any obvious presence of any major merging event, however, the smoothness of the disk could indicate a minor past merging event.
