The galaxy appears to be a relatively smooth, centrally concentrated object with a slight elongation. Its color profile exhibits a yellowish-orange hue, suggesting an older stellar population dominating its light output, with less active star formation present. The galaxy's morphology leans towards elliptical, with a generally round shape but some evidence of a deviation from perfect circularity. There does not appear to be major disturbances or a significant merger event affecting it, although some low-level asymmetries may suggest a minor interaction in its past.
