The galaxy presents as a single, fairly symmetrical object. It exhibits a smooth, elliptical morphology, lacking any readily discernible spiral arm structure or prominent dust lanes. There is a notable concentration of light towards the center, suggesting a dense galactic nucleus. The color gradient transitions from a yellowish core to a redder halo, potentially indicative of an older stellar population. It appears to have undergone minimal recent interaction or disturbance, showing no signs of tidal tails or significant morphological irregularities. The object is relatively compact, exhibiting a uniform structure without substructures.
