This galaxy presents a moderately bright, but complex morphology. The central region exhibits a highly luminous core, appearing almost saturated in the image. This core is surrounded by a fainter, more diffuse halo of light. 

There is evidence of disturbed morphology within the outer regions of the galaxy. Some asymmetry is observed, with a slight elongation or distortion visible on one side. The color gradients suggest varying stellar populations or dust content across the galaxy, with bluer tones in the outer regions potentially indicating ongoing star formation. Overall, the galaxy does not appear to be a classic elliptical or spiral, but rather something more irregular or potentially interacting. The overall impression is of a system that has experienced some form of disruption.
