The galaxy presents with a morphology that appears to be undergoing significant interaction or a merger. The structure is neither distinctly elliptical nor spiral, appearing as a disturbed system with a primary, brighter component and a secondary, slightly less luminous component. The primary component exhibits a yellowish-white core, suggesting an older stellar population, possibly dominated by evolved stars. The secondary component is more reddish in hue, which might indicate a more recent burst of star formation or a dust-obscured region. There is an asymmetry in the overall shape, indicative of gravitational disturbances. Faint tidal features or extended halos are not clearly visible, but the irregular shape implies that these features might be present but are below the detection threshold.
