The galaxy presents as a largely smooth, elliptical morphology with a high degree of central concentration. Its color is a yellowish-orange, suggesting a stellar population dominated by older, redder stars. There is no evidence of spiral arms or a prominent disk structure. The galaxy appears relatively undisturbed, with no obvious signs of tidal features or ongoing mergers. It seems well-defined with a round shape, although with what appears to be a slight elongation on one side. The galaxy possesses a substantial mass and has a relatively low star formation rate, indicating that the majority of star formation occurred in the past.
