The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The core region exhibits a yellowish-white hue, suggesting an older stellar population. The outer regions fade into a more diffuse, slightly bluer light, indicating some presence of younger, hotter stars, though less prominent than the central population. The galaxy is elongated, appearing somewhat oblate, with no discernible spiral arm structure or significant dust lanes. There is a slight indication of a faint halo or extended stellar envelope surrounding the galaxy. Overall, the galaxy seems to be an intermediate-mass system, undergoing limited star formation. Subtle disturbances are potentially present, without significant morphological signs of a recent major merger.
