The galaxy presents as an elliptical morphology, exhibiting a generally smooth and concentrated light profile. The core is very bright and compact, suggesting a high density of stars in the central region. The galaxy appears relatively undisturbed, with no obvious signs of tidal interactions or ongoing mergers. There is a slight elongation along one axis, but it is mostly round. Color gradients are subtle but visible; the central region has a slightly redder hue, potentially indicating an older stellar population, while the outer regions have a relatively green tint, possibly reflecting younger stars or a lower metallicity. The overall color suggests intermediate star formation activity. There is no evident dust lane or distinct spiral structure.
