The galaxy presents as a relatively smooth, elliptical-like object with a centrally concentrated brightness profile. It appears yellowish-white, potentially indicating an older stellar population. There's a slight elongation, suggesting it is not perfectly spherical. No prominent spiral arms, dust lanes, or other distinguishing features are immediately apparent. The outer edges are quite faint and diffuse, fading into the background sky. The smooth morphology suggests minimal ongoing merger activity or significant star formation within the observed timeframe.
