This galaxy exhibits a largely elliptical morphology with a smooth light distribution. A concentrated, luminous core is present, characterized by a yellow-orange hue indicative of an older stellar population. The outer regions of the galaxy appear more diffuse, transitioning to a greenish tint, possibly indicating the presence of a younger stellar population or ongoing star formation, though at a relatively low rate. There is no prominent disk structure visible, nor any indication of major mergers or strong tidal disturbances. The overall shape is generally round, with no significant elongation or asymmetries observed. The galaxy appears to be a relatively massive system.
