The galaxy exhibits a somewhat elongated morphology, appearing as an irregular and diffuse structure. The central region is characterized by a bright and relatively compact core. Moving outward from the core, the galaxy presents a fainter, extended halo or disk. The light distribution within the outer regions of the galaxy appears uneven, suggesting possible asymmetries or tidal disturbances. A slight color gradient is observed, with bluer hues concentrated primarily towards the outer regions. This could indicate ongoing star formation in these areas. Overall, the galaxy displays a generally distorted structure, indicating potential interactions or past merger events, although without clear signs of an ongoing major merger event.
