The galaxy presents an elliptical morphology, exhibiting a smooth, featureless appearance in the central region. A notable concentration of light is observed at the core, gradually decreasing in intensity towards the outer edges. There is a slight deviation from perfect circularity, leaning toward an intermediate shape. The primary color is yellow, suggesting an older stellar population. At the bottom edge of the galaxy, a separate clump of red-shifted light can be observed. This could be a minor interaction or a region of concentrated star formation. No prominent spiral arms or significant dust lanes are discernible within the image. Overall, the galaxy seems to have a considerable mass and a relatively low rate of current star formation.
