The galaxy presents as a relatively smooth, elliptical object. It appears to have a primarily spheroidal morphology with little discernible disk structure. The central region exhibits a yellowish hue, potentially indicating a population of older stars or dust obscuration. There is evidence of potential ongoing or recent merger activity with other galactic structure as the surrounding region seems disturbed. A distinct blue region is observed, suggesting areas of recent star formation, potentially triggered by the merger. Overall the galaxy has a moderate redshift with a significant stellar mass and what appears to be low star formation overall.
