The galaxy presents as a relatively smooth, centrally concentrated object. It appears elliptical, with a high degree of circularity. The color profile suggests an older stellar population with a predominantly yellow-orange hue in the central bulge, fading to bluer shades in the outer regions. There is no strong evidence of spiral arms, bar structures, or significant dust lanes. The overall morphology indicates an early-type galaxy, likely an elliptical or lenticular, with minimal signs of active star formation or recent merger activity. Small disturbances may be present but seem minor.
