The galaxy presents as a relatively smooth, elliptical structure. Its core exhibits a concentrated, bright yellow-orange hue, indicating a likely older stellar population and minimal active star formation in the central region. The outer regions display a gradual fading in intensity, transitioning to a greenish-blue tint. This suggests the presence of a younger stellar population and ongoing star formation in the galactic outskirts, though not substantial. There is a faint distortion on the edge of the disk which may point to a minor merger.
