The galaxy presents as a faint, elongated, disk-shaped structure viewed nearly edge-on. The central bulge appears rounded and is subtly brighter than the rest of the disk, indicating a concentrated stellar population. The disk exhibits a relatively smooth texture, with minimal visible dust lanes or distinct spiral arm features. There may be some signs of a minor disturbance, though this is not certain. Overall, this galaxy appears to be a late-type, rotating system, with relatively little star formation activity.
