The galaxy presents as a centrally concentrated object, appearing largely smooth in morphology. It exhibits a dominant yellowish-orange hue in its core, suggesting an older stellar population. The galaxy's shape approximates a rounded profile, though a slight deviation from perfect circularity is observed. Faint extensions are visible, possibly indicative of tidal interactions or minor disturbances. The absence of distinct spiral arm structures or prominent dust lanes supports the interpretation of a more evolved system. Overall, the galaxy appears to be a relatively massive system with a moderate redshift, consistent with an elliptical morphology.
