The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits a largely elliptical morphology, presenting a high degree of circularity with minimal elongation. No distinct spiral arms or bar structures are discernible. The galaxy has a bright, compact core that diminishes gradually in intensity outwards. There are no signs of major mergers or significant tidal disturbances. The light appears dominated by older stellar populations, suggesting a lack of ongoing, intense star formation. The overall color is consistent with evolved stars. It may be a dwarf elliptical galaxy in the local universe.
