The galaxy presents as a largely smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing quite rounded in shape. The color profile suggests an older stellar population, with a yellowish hue dominating the central bulge region. There's little evidence of distinct spiral arms or significant dust lanes. No signs of major mergers or tidal disturbances are visible. The faintness of the outer regions suggests low levels of on-going star formation.
