The galaxy exhibits a somewhat disturbed morphology, possibly indicative of an ongoing or recent interaction. A disk-like structure is present, oriented approximately edge-on relative to our line of sight. The disk appears relatively thick, with a noticeable degree of internal structure.  There's an indication of brighter, possibly star-forming regions concentrated within the disk. The overall color suggests moderate ongoing star formation activity. Some disturbances are evident, potentially linked to a minor merger event or tidal interactions.
