The galaxy presents as a centrally concentrated object with a generally smooth, elliptical morphology. There is a slight elongation visible, deviating minimally from a perfectly circular shape. The color profile suggests an older stellar population, appearing redder in overall color. The galaxy exhibits a lack of distinct spiral arm structures or prominent dust lanes. There are no obvious signs of recent major merger activity, though a subtle asymmetry could suggest a minor interaction or disturbance. The galaxy's light is relatively concentrated towards the center, indicating a dense core. The object does not display any pronounced star-forming regions within the observable spectrum.
