The galaxy presents a complex morphology, possibly indicative of an ongoing or recent merger event. The dominant feature is a concentrated central bulge exhibiting a yellowish-white hue, suggesting an older stellar population. Extending from this core are fainter, more diffuse structures. Patches of bluer light are observed, potentially indicative of ongoing star formation regions embedded within the galactic body. There also appears to be what could be two galaxies interacting within this image. This merging may cause tidal forces, with visible signs of disturbance.
