The galaxy presents an elliptical morphology, appearing largely smooth and featureless. The core region exhibits a concentrated, reddish hue, suggesting an older stellar population, perhaps dominated by red giant stars. Moving outward from the core, the color transitions to a greenish-blue halo. This may indicate the presence of some younger, hotter stars, and potentially ongoing, but likely limited, star formation in the outer regions. The galaxy exhibits a moderate degree of ellipticity, appearing more elongated than perfectly circular. There is no strong evidence of spiral arm structure or significant dust lanes visible in this image, further supporting its classification as an elliptical galaxy. There are no obvious signs of tidal disturbances or interactions with neighboring galaxies, indicating it is a relatively isolated system.
