The observed galaxy exhibits a morphology consistent with a disturbed spiral galaxy, potentially undergoing a merger event. The central region presents a bright, moderately sized bulge. A complex disk structure is present, displaying evidence of both spiral arm fragments and significant morphological distortions.

A noticeable tidal tail extends outward from the main galactic body. This is indicative of gravitational interaction with another galaxy, past or present. Irregularities are observed within the disk, implying a disruptive event that could trigger heightened star formation in these regions. The overall colour profile suggests a mix of stellar populations; bluer regions likely correspond to areas of active star formation, whereas redder areas likely represent older, more evolved stellar populations. The lack of a well-defined bar structure is apparent.
