The galaxy appears to be elliptical in shape, exhibiting a smooth and featureless morphology. Its light is concentrated towards the center, displaying a bright, yellowish-orange core that likely indicates an older stellar population. There is no obvious spiral arm structure or distinct dust lanes visible. The lack of prominent features suggests a quiescent galaxy with low ongoing star formation. The galaxy's color is slightly redder compared to typical spiral galaxies, which further indicates a more evolved stellar population. There is no clear evidence of any major mergers or significant tidal disturbances. The galaxy appears relatively isolated in this image.
