The galaxy presents as a single, relatively smooth, and centrally concentrated object. It exhibits a moderate degree of ellipticity, appearing somewhat flattened rather than perfectly circular. The light distribution shows a strong concentration toward the core, with a gradual decrease in intensity outwards. There is an apparent lack of distinct spiral arm structures or prominent dust lanes. The galaxy's color is predominantly yellow/orange, suggesting an older stellar population with fewer young, massive stars. No obvious signs of active galactic nuclei activity or major mergers are discernible. The galaxy likely resides at an intermediate distance, given the observed redshift and apparent size.
