The galaxy appears as a flattened spheroid with a relatively high surface brightness, suggesting an elliptical morphology when accounting for possible inclination. The core region exhibits a bright, concentrated luminosity, indicating a potentially dense stellar population or active galactic nucleus. Evidence of faint, extended features surrounding the central region is visible. There is a possibility of a tidal interaction or minor merger based on distortions of the outer halo of the galaxy. A color gradient is observed, with the central region appearing bluer.

