This galaxy exhibits a morphology indicative of a system undergoing significant interaction or disturbance. The central region is characterized by a bright, diffuse bulge, possibly masking a dense galactic nucleus. A faint, extended disk is present, although its structure appears irregular and disrupted. There are indications of tidal features or streamers extending outward from the main galactic body, suggesting gravitational interaction with another galaxy or past merger events. Color variations within the disk suggest varying stellar populations, with bluer regions potentially indicating ongoing star formation. The overall appearance of the galaxy is not smooth, with evidence of clumpy structures and asymmetries, further supporting its classification as an interacting or post-merger system. Some dust lanes are visible, although they are not highly prominent. The galaxy's morphology is suggestive of a complex evolutionary history involving external influences.
