The galaxy presents as a relatively smooth object, potentially of an elliptical nature, with minimal discernible structure within the observed light. The galaxy is roughly elliptical in shape, appearing more elongated than circular. There is a bright, central region that fades gradually toward the edges. The color profile seems homogenous across the galaxy, with the primary contribution being in the green and red wavelengths. The red shift value suggests that this is a reasonably distant galaxy. Overall, the galaxy lacks significant signs of active star formation or significant recent merger events.
