The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a distinct bar structure. The galaxy's color profile suggests a relatively old stellar population, exhibiting a yellowish-red hue indicative of evolved stars. There is a slight elongation in its shape, hinting at possible tidal interactions or an internal asymmetry, but the overall structure remains largely undisturbed. The galaxy appears to be a significant mass, but is currently exhibiting very little to no active star formation. There might be very small signs of minor disturbances.
