The galaxy presents as a centrally concentrated object with a smooth, somewhat diffuse morphology. There's an apparent lack of defined spiral arms or a prominent galactic disk. The light is primarily concentrated in a central bulge, fading gradually toward the edges of the galaxy. A slight elongation is noticeable, deviating from a perfectly circular shape. Color gradients suggest a mix of stellar populations. The central region exhibits a relatively brighter and potentially redder hue. While the galaxy appears mostly undisturbed, subtle irregularities might suggest minor gravitational interactions or internal activity. The overall impression is that of a mature galaxy, possibly an elliptical or lenticular type, displaying a largely quiescent state of star formation.
