The galaxy presents as a somewhat amorphous, elliptical structure. Its core region appears denser and exhibits a bluer hue, which could indicate a population of younger, hotter stars, and ongoing or recent star formation. The outer regions of the galaxy fade gradually into the background, with a more diffuse distribution of stellar populations. The overall shape is largely smooth, lacking any clear spiral arm structures or prominent dust lanes. There is a slight flattening, giving it a lenticular appearance, though not as obviously structured as a typical spiral galaxy. The primary axis appears to be oriented close to vertical in the image.
