The galaxy presents as a relatively small, elliptical-like structure. The central region exhibits a higher surface brightness, appearing nearly uniform in color. There is a faint, extended halo of light surrounding the core, suggesting a gradual decrease in stellar density with increasing radius. The overall color profile appears slightly redder, potentially indicating an older stellar population. There is some evidence of a possible tidal feature, but the morphology is predominantly smooth and undisturbed, suggesting that there are no major recent merger events. The color distribution is consistent with it being an early type galaxy.
