The galaxy presents as a highly elongated, disk-shaped structure viewed edge-on. The central region exhibits a pronounced bulge of concentrated light, appearing yellowish, suggestive of an older stellar population. The disk appears relatively smooth with little visible structure such as spiral arms or dust lanes. The outer regions of the disk gradually fade into the background, indicating a relatively sharp boundary. There is little evidence of ongoing star formation from visual inspection. The overall morphology suggests a relatively quiescent disk galaxy, possibly of late-type classification, with no major disturbances detected.
