The galaxy presents as a largely smooth, elliptical-like structure, exhibiting a relatively round morphology. The central region is noticeably brighter and appears yellowish, potentially indicating an older stellar population. There may be a minor disturbance in the morphology or an indication of a minor merger event. The overall light distribution suggests a concentration towards the center, consistent with an early-type galaxy. There is a small concentration of light slightly separated from the main body, potentially the source of the observed morphological disturbances. This galaxy appears relatively massive with a low star-formation rate. The structure is indicative of a galaxy that is nearing the end of its formation process.
