The galaxy appears to be composed of two distinct components: a more concentrated, yellow-orange central region and a fainter, bluer region situated inferior to the central structure. The central region exhibits a relatively smooth morphology, suggesting an older stellar population or a spheroidal structure. In contrast, the bluer region shows a more diffuse appearance, potentially indicative of ongoing star formation. There is a suggestion of tidal features or asymmetries emanating from the main body, hinting at past or ongoing gravitational interactions. Overall, the galaxy presents an interesting morphology warranting further investigation into its formation history and evolutionary processes.
