The galaxy presents as an elliptical or lenticular system, exhibiting a smooth, centrally concentrated luminosity profile. The core region displays a bright, concentrated nucleus, suggesting a substantial stellar density. The overall color index appears relatively uniform across the galaxy, trending towards the blue end of the spectrum. The morphology suggests a system that may have undergone significant dynamical relaxation. There is a slight indication of tidal disturbances, suggesting the possibility of previous interactions or mergers. The lack of strong spiral arm features or prominent dust lanes indicates that the star formation rate is relatively low. The galaxy's shape is elongated, resembling an elliptical shape. While there isn't any single major disturbance, there is a slight suggestion of some disturbances.
