The galaxy presents as a relatively smooth, elliptical structure. Its light profile suggests an older stellar population, with a concentration of light towards the core. The galaxy appears largely undisturbed, though there are indications of minor asymmetry or possible tidal features in its outer regions, hinting at past interactions. There is no pronounced spiral structure or distinct dust lanes visible. The overall color suggests a redder hue, consistent with a population of evolved stars and a low rate of current star formation. The galaxy's apparent size is small, indicating a substantial distance.
