The galaxy appears as a concentrated, somewhat diffuse object. It exhibits a generally smooth morphology, lacking prominent spiral arms or a well-defined disk structure. The central region presents a bright, yellow-ish core, suggesting a concentration of older stellar populations. Moving outward from the core, the galaxy appears to fade into a more indistinct halo. There is some slight elongation to the overall shape, but it is mostly round. There is no obvious indication of major disturbances or ongoing mergers in this image.
