The galaxy presents a complex morphology, exhibiting characteristics suggestive of an ongoing or recent merger. The central region displays a diffuse, yellowish glow, potentially indicating an older stellar population and/or dust obscuration. Extending from this core are fainter, blueish tinged areas, perhaps associated with pockets of more recent star formation. The overall structure appears significantly disturbed and asymmetric. The shape is irregular, deviating substantially from a regular elliptical or spiral form. Tidal features, such as faint plumes or extended halos of stars, are not clearly discernible in this image, though the disturbed morphology itself could be a result of tidal interactions. Further spectroscopic analysis is required to fully understand the stellar populations, gas content, and kinematics of this system, and to confirm the presence and nature of any merger activity.
