The galaxy presents as a smooth, elliptical-like object with a discernible bulge. The central region exhibits a yellowish-red hue, possibly indicating an older stellar population. Proceeding outwards from the core, a green tint becomes apparent in what would resemble the disk; the green tint could be indicative of ongoing, low-level star formation. The overall shape suggests a system that is neither perfectly round nor highly elongated, showing a shape somewhere in between. There appears to be no obvious major merger events disturbing the overall structure, but subtle irregularities or minor disturbances cannot be ruled out.
