The galaxy presents as a somewhat diffuse and indistinct object. It displays a generally elliptical morphology, appearing largely smooth with a concentrated central bulge. Faint color gradients are visible within the galaxy, shifting from yellow-orange in the core to slightly redder hues in the outer regions, suggesting a population of older stars. There are indications of a faint disk structure viewed edge-on, bisecting the galaxy. Evidence suggests some merging might be occurring, possibly a minor disturbance or an ongoing merger event. There's no clear structure or defined spiral arms evident in this image.
