The galaxy appears as a centrally concentrated object with a relatively smooth light distribution. There is a slight elongation apparent, although the overall shape is generally round. The color is primarily a yellowish-white, suggesting a dominant population of older stars, although a hint of bluer light is present in some regions indicating the presence of some younger stars. There are no distinct spiral arms or a well-defined disk structure visible; the galaxy has an amorphous shape. There is no evidence of strong tidal features or ongoing major mergers, though some minor disturbances or interactions cannot be completely ruled out based on the image alone.
