The galaxy presents a complex morphology, possibly indicative of an ongoing interaction or merger event. The central region appears relatively smooth and concentrated with a yellowish hue, suggesting a population of older stars and possibly a bulge component. Extending from this central region are fainter, bluer regions.

These bluish components are suggestive of active star formation regions and younger stellar populations. A distinct plume or tail-like feature is observed extending from the main body of the galaxy, which could be tidal debris resulting from a gravitational interaction. A separate, smaller region appears detached from the main galaxy, further supporting the possibility of a disrupted structure. The overall shape deviates significantly from a regular spiral or elliptical morphology, indicating a disturbed or irregular structure.
