The galaxy presents a morphology indicating a system undergoing a significant interaction or merger. Its overall shape is irregular and elongated, deviating substantially from a regular elliptical or spiral form. The central region appears disturbed, showing a brighter, somewhat amorphous core with evidence of multiple luminous knots or condensations. Faint extensions or tidal tails are present, one more prominent than the others, suggesting gravitational disruption due to the interaction with another galaxy or object. Color variations within the galaxy are apparent, with bluish regions possibly indicating areas of recent star formation, juxtaposed with yellower regions indicating older stellar populations. The asymmetry and disrupted morphology strongly suggests ongoing gravitational disturbance.
