The galaxy presents as an elliptical morphology, though with some features suggesting a disk or disturbance. A central bulge is visible, appearing relatively bright and concentrated. Diffuse blue light extends outwards from the bulge, indicating the potential presence of younger stars and star formation regions. The edges of the galaxy are indistinct, fading into the background sky. Possible minor disturbances are visible, such as irregularities in its shape and extensions of light, though these could also be artifacts. There is no evidence of ongoing major merger activity in this image. 
