The galaxy appears as a slightly elongated, centrally concentrated object. The light is relatively smooth and diffuse, showing no prominent spiral arms or distinct features. There may be some internal structure visible within the central region, but the resolution is not high enough to determine its nature. The galaxy has a distinct blue hue, suggesting ongoing or recent star formation, which corresponds with the blue-shifted wavelength. The absence of strong tidal features or other obvious signs of interaction suggests that it is a relatively isolated system that has not had major disturbances recently.