The galaxy presents as a disk galaxy, oriented approximately edge-on relative to our line of sight. A prominent central bulge is observed, exhibiting a yellowish-white hue suggestive of an older stellar population. The disk appears asymmetrical and is relatively well-defined. Evidence of spiral arm structure is subtle but present. Patches of blue light indicate regions of active star formation within the disk. There does not appear to be any ongoing major merging activity, though a possible minor disturbance can not be ruled out. The galaxy exhibits an overall smoothness.
