The galaxy presents a smooth, elliptical morphology. Its color profile exhibits a gradient, transitioning from a predominantly yellow core to redder hues at its periphery. This color suggests an older stellar population. The galaxy is elongated, with the major axis significantly larger than the minor axis. No distinct spiral arm structures or prominent dust lanes are discernible. There is a faint blueish halo enveloping the galaxy. Overall, the galaxy appears relatively undisturbed, lacking any major signs of ongoing mergers or tidal interactions, although subtle disturbances can not be ruled out.