The galaxy presents a complex morphology, potentially indicative of an ongoing or recent interaction or merger event. It appears to be composed of multiple distinct luminous regions, with a dominant, relatively smooth component and a more disturbed section. The prominent smooth component appears somewhat round in projection. This section emits strongly across the observed optical bands, with a relatively even color distribution suggestive of a well-mixed stellar population.

To the right of the smooth component are two distinct regions that appear less uniform and have a different color, skewed towards redder wavelengths. The morphology in this part of the system appears less relaxed than the smooth component, suggesting that this section may be the result of a recent accretion or merger event.

Evidence of a possible tidal tail or other extended structure is not clearly visible in this imaging, but the overall irregular morphology warrants further investigation into its kinematic and stellar population properties to confirm its evolutionary state.
