The galaxy presents as a diffuse object with a slightly elongated shape. There is a notable central concentration of light, appearing yellowish-orange, suggesting an older stellar population is dominant in the core. Surrounding the central region is a fainter, more irregular distribution of light, exhibiting a bluish tint in some areas. The overall morphology indicates a system undergoing, or having recently undergone, a significant interaction or disturbance. Evident distortions in the outer regions support the possibility of ongoing tidal interactions or a recent merger event. These interactions may be the cause of regions of younger, bluer stars.
