The galaxy appears to be a relatively smooth, elliptical-like structure. Its core region exhibits a high degree of luminosity, appearing nearly spherical and concentrated. The light smoothly decreases in intensity towards the edges. There may be a very faint hint of a disk. No signs of major mergers or disturbances are apparent in the image, although some minor irregularity cannot be ruled out. The color profile suggests the presence of an older stellar population, evidenced by the redder hues, with possibly some younger, bluer stars mixed throughout the galaxy, but primarily concentrated in the center of the galaxy. The structure is consistent with an early-type galaxy.
