The galaxy appears to be a relatively smooth, elliptical or lenticular system. Its overall color profile suggests a dominant population of older stars, with a noticeable central concentration of light that is yellowish/white. The galaxy is largely featureless, lacking prominent spiral arms or strong dust lanes. There may be some slight, faint hints of a disk component, but this is not pronounced. Its shape is nearly round, with only very slight elongation. There are no signs of major ongoing mergers or significant tidal disturbances affecting the galaxy's structure. It appears to be a relatively isolated and evolved galaxy.
