This galaxy presents as a single luminous core with significant surrounding nebulosity extending beyond the bright central region. A prominent, somewhat linear, feature extends outward from the core. The galaxy's overall morphology suggests a complex system, possibly undergoing interactions or exhibiting significant internal dynamics. The central region exhibits a high concentration of light, appearing almost stellar in nature, which could indicate the presence of an active galactic nucleus or a very dense stellar population. The outer regions appear less structured and more diffuse, forming a halo-like structure that fades into the background sky. There is evidence of disturbed morphology suggestive of possible past or ongoing merger events, exhibiting a deviation from a typical smooth elliptical or spiral structure.
