The galaxy presents as a roughly elliptical structure, with a smooth, diffuse light distribution. The core region exhibits a relatively high surface brightness. The light appears to be bluer in the central regions. Moving outward from the core, the light reddens slightly, with the outer edges fading into the background sky level. There is no strong evidence of spiral arm structure, rings, or dust lanes visible in this image. The overall morphology suggests a galaxy without any major merger events or tidal disturbances, indicating that it has not recently interacted with another galaxy. The galaxy displays a significant ellipticity, which may be indicative of the viewing angle or could reflect an intrinsic triaxial shape.
