The galaxy presents as a generally smooth object, potentially an elliptical. The core exhibits a high surface brightness, with a gradual decrease in luminosity outward. The shape appears to be somewhat elongated, though not extremely so, showing a moderate ellipticity. There are no visually discernible spiral arm structures or dust lanes. Faint, diffuse light extends outward from the central region, fading into the background sky. The color profile indicates a possible reddish hue, typical of older stellar populations. There is no evidence of any significant tidal features or ongoing merger activity.
