The galaxy presents as a generally smooth, centrally concentrated object. Its overall morphology appears elliptical, approaching circularity, with no prominent features such as spiral arms or a distinct disk component readily apparent. The light is dominated by warmer colors, trending towards yellow, indicating a population of older stars within. The galaxy exhibits a luminous core which decreases in intensity gradually outwards. This intensity profile lacks sharp edges, further suggesting an older, well-mixed stellar population. There is a faint hint of subtle irregularities at the outer edges, however, this is more likely due to noise in the image rather than actual disturbances. The observed color and smoothness suggest a lack of ongoing major star formation, consistent with a classification as an elliptical galaxy. 
