The galaxy presents as a somewhat elongated structure, exhibiting a smooth, elliptical-like morphology. It appears to have a diffuse, extended halo or envelope of light surrounding a brighter central region. The color profile suggests a relatively evolved stellar population, with a redder hue overall. There is a hint of a possible disk-like component oriented approximately horizontally, as viewed in the image, although it is not sharply defined. Some minor disturbances may be present within the galaxys structure and this structure is likely not undergoing major merging activity.
