The galaxy presents as a relatively smooth, elliptical-like structure with a high degree of central concentration. Its morphology appears undisturbed, with no obvious signs of tidal features or major mergers. The light is dominated by redder wavelengths, suggesting an older stellar population. There is a slight elongation, indicating it is not perfectly circular, with a position angle that can be estimated by the image. There is a possible faint disk present. There appear to be no distinct spiral arms or prominent dust lanes visible in this image.
