The galaxy presents as a largely featureless, elliptical morphology with a smooth light distribution. The galaxy exhibits a concentrated central bulge, which appears reddish, suggesting an older stellar population. Moving outward from the core, the color shifts towards a yellow-green hue, possibly indicating a slightly younger stellar population or a minor component of ongoing star formation, although at a low rate. The galaxy appears largely undisturbed, showing no obvious signs of recent major merger activity or significant tidal distortions. There is only a slight elongation and little to no evidence of spiral arms. The lack of prominent dust lanes and the smooth light profile further supports its classification as an elliptical galaxy. Overall, the galaxy seems to be a relatively evolved system with minimal current star formation.
