The galaxy presents as a primarily smooth, elliptical-like structure. The central region exhibits a concentrated, bright luminosity, suggesting a significant stellar population density. Fainter, diffuse light extends outwards from the core, indicating a gradual decrease in stellar density with increasing radius. A slight elongation or asymmetry is observed in the outer regions of the galaxy. A faint blue tail can be seen trailing off to one side of the galaxy. Overall, the galaxy appears to be relatively isolated and undisturbed.
