The galaxy appears to be an elliptical type, exhibiting a generally smooth and concentrated light profile. The core region presents a bright, yellowish-white hue, indicative of an older stellar population. There is a subtle shift in color from the central core to the outer regions, with a slight reddening potentially suggesting the presence of dust. The galaxy is somewhat elongated, deviating slightly from a perfectly circular shape. There is little evidence of significant spiral arm structures or prominent star-forming regions. Some minor disturbances cannot be ruled out.
