The galaxy appears to be a field galaxy, exhibiting a distinct morphology. The central region is bright and concentrated, likely indicating a significant stellar population or an active galactic nucleus. Surrounding the core, there is a fainter, more diffuse structure. The shape is generally rounded but shows some irregularities, suggesting the potential for past or ongoing interactions. There are hints of spiral arm-like structures, though they are not well-defined. One side is more heavily weighted than the other. There is likely some distortion of its shape and some minor disturbance occurring.
