The galaxy presents as a luminous, centrally concentrated object with an apparent smooth morphology. A distinct nucleus emits a bright, yellowish light, suggesting an older stellar population in this region. The overall color profile transitions outwards to a bluer hue, hinting at the presence of younger stars or ongoing star formation in the outer regions of the galaxy. There is a slight asymmetry present, which may be an indication of minor disturbances in the gravitational field. The galaxy exhibits an elliptical shape, deviating slightly from a perfect circle. The galaxy appears relatively isolated with no obvious signs of major interactions.
