The galaxy presents a complex morphology suggestive of an ongoing or recent interaction. A dominant central region exhibits a yellowish-orange hue, possibly indicating a population of older stars and/or significant dust obscuration. This region appears somewhat irregular, lacking a clear spiral or elliptical structure. Emanating from this central area are fainter, diffuse structures exhibiting a bluer tint. These features may be indicative of younger stellar populations or ongoing star formation activity triggered by the interaction. 

One distinct, bright blue region is present on the periphery of the galaxy. This localized concentration of blue light strongly suggests an active star-forming region, possibly a giant HII region or a young star cluster. The overall light distribution is not uniform. There is asymmetry, further supporting the hypothesis of tidal disturbances and gravitational interactions shaping the galaxy's structure. Dust lanes are not clearly visible but cannot be ruled out due to the limited resolution of the image. 
