The observed galaxy presents as a somewhat compact object, roughly estimated to be a few arcseconds in diameter. It displays a complex morphology. A bright, central region dominates the galaxy's appearance. Surrounding the central core, there are indications of fainter, more diffuse structures. The central luminosity is intense, potentially hinting at a dense stellar population or active galactic nucleus. Distinct color variations are observed across the galaxy. The central region appears relatively neutral in color, while more extended regions show bluer hues. A possible tidal tail is indicated, but this is faint. Redder structures are also noted along its edge, suggesting regions of dust obscuration or older stellar populations. Based on the apparent irregularity of the structure, the galaxy may have undergone some sort of recent tidal or merger activity.
