The galaxy presents as a primarily smooth, elliptical structure. There is a suggestion of some minor morphological disturbance, with some light being pulled to the left-hand side. The central bulge exhibits a yellow-orange hue, suggesting a population of older stars. This is in stark contrast to the hint of blue light on the other side, indicative of younger, hotter stars. There is very little evidence of prominent spiral arms or a well-defined disk structure; overall, the appearance suggests a galaxy that is relatively evolved, but is also interacting with another galaxy on the left-hand side.
