The galaxy presents as a relatively smooth, elliptical structure with a bright, concentrated core. It exhibits a near-spherical morphology, lacking any prominent spiral arms or disk features. The light distribution appears uniform with a noticeable absence of dust lanes or significant irregularities in its shape, hinting towards an older stellar population. No signs of recent or ongoing merger activity, such as tidal tails or disturbed morphology, are evident, indicating a relatively isolated and undisturbed system. The galaxy has a yellow-red hue.