The galaxy presents as a relatively smooth, elliptical form with a high degree of central concentration. Its color profile tends toward the redder end of the spectrum. There is little apparent structure such as spiral arms or distinct dust lanes. The galaxy appears moderately luminous, indicating a significant stellar population. The lack of distinct features suggests a more evolved system with a low ongoing star formation rate. Faint hints of possible minor disturbance or tidal features are present in the outer edges of the galaxy, warranting further investigation into its potential interaction history.
