This galaxy exhibits an elliptical morphology, appearing largely spheroidal in shape. The galaxy appears generally smooth in texture with little evidence of strong spiral arm structures or significant dust lane obscuration. The color profile suggests an older stellar population, exhibiting a reddish-yellow hue with a subtle change in color from core to edge. This indicates potentially less ongoing star formation with a possible population of evolved stars, particularly towards the galactic center. There is potential indication of either a minor gravitational interaction or early stage merger event due to the slight asymmetry of the galaxy's shape.
