The galaxy appears as a somewhat elliptical, relatively smooth structure with a concentrated central bulge. There is a color gradient from the center outwards, with the core exhibiting a yellowish hue, transitioning to a bluish-white color in the outer regions. There is a slight indication of disk-like morphology but with minimal defined spiral structure; it presents as more of a flattened spheroid. The overall light distribution suggests a lack of ongoing major mergers or strong tidal disturbances, although a hint of irregularity cannot be ruled out. The galaxy is moderately luminous. The light profile suggests moderate levels of star formation activity, more dominant in the blue outer regions.
