The galaxy presents as an elliptical system, elongated in shape, with a smooth, diffuse light distribution and no apparent spiral arm structure or prominent dust lanes. The core region exhibits a bright, concentrated luminosity, suggesting a high density of stars or potentially an active galactic nucleus, though higher resolution imaging would be required to confirm this. The overall color gradient transitions from a yellowish-white core to a slightly bluer hue in the outer regions, which could indicate the presence of a younger stellar population at the periphery, or it could be an artifact of the imaging. There are no obvious signs of tidal interactions or major disturbances, such as tidal tails or asymmetric features. The galaxy displays a relatively high degree of smoothness and light concentration.
