The galaxy presents as a relatively smooth, elliptical or lenticular structure. Its light is concentrated towards the center, displaying a pronounced bulge with a yellow-orange hue, suggesting an older stellar population. There is a lack of clearly defined spiral arms, indicating a dearth of active star formation. The overall shape appears somewhat rounded, with a subtle elongation. There is no obvious signs of recent or ongoing major merger activity, such as tidal tails or strong morphological distortions, though minor disturbances cannot be ruled out. The color gradient moves subtly to a slightly bluer hue outside the concentrated center.
