The galaxy presents as a relatively smooth, elliptical structure with a centrally concentrated light profile. Its overall shape is generally rounded, with a slight elongation that deviates minimally from a perfect circle. There is no distinct spiral arm structure visible. The color appears to be a somewhat uniform blue-white across the galaxy's body, implying the presence of a moderate population of younger, hotter stars, although older stellar populations likely dominate. There are no obvious signs of ongoing major merger activity. The galaxy is of moderate size. There are no visible tidal tails, plumes, or strong distortions in its overall morphology, indicating it is relatively undisturbed.
