This galaxy exhibits a complex morphology, suggestive of an ongoing or recent merger event. The primary body of the galaxy appears diffuse, with a generally smooth appearance punctuated by two brighter, more concentrated regions that could be the remnants of galactic cores. These regions are characterized by a yellowish-white color, potentially indicative of older stellar populations.

The overall shape is somewhat elongated, but significantly disturbed. Patches of redder emission are scattered throughout the galaxy, possibly indicating regions of dust obscuration or recent star formation. A faint, extended halo or tidal feature can be tentatively identified, further supporting the hypothesis of a merger or tidal interaction. The galaxy does not present a well-defined spiral or elliptical structure, and it shows clear signs of morphological irregularity.
