The galaxy presents a largely smooth, elliptical morphology. There is a dominant central bulge exhibiting a yellowish hue, likely indicative of an older stellar population. The galaxy appears somewhat flattened, displaying an intermediate ellipticity, not quite spherical but also lacking a distinct disk structure. Faint, diffuse extensions of light surround the central bulge, suggesting a halo component. There's no strong evidence of spiral arms or significant dust lanes; the overall structure is relatively featureless. The galaxy's color profile suggests a red sequence galaxy. There may be signs of minor disturbance but further observations are needed to confirm.
