The galaxy presents as a structured system with a distinct, bright core. The core region is characterized by a smooth, concentrated luminosity profile, suggesting an older stellar population. Extending from this central region is a fainter, more diffuse structure. The morphology suggests possible interaction or merger activity, with evidence of tidal features or distortions in the outer regions. There appears to be an extended tail or plume of stellar material emanating from the main body of the galaxy. The color gradient within the galaxy indicates variations in stellar populations and dust content. The central bulge displays bluer colors, potentially indicating recent or ongoing star formation, while the outer regions exhibit redder hues, suggestive of older stellar populations. Overall, the galaxy appears to be in a state of dynamic evolution, potentially undergoing transformation due to internal processes or external interactions.
