This galaxy presents as a generally smooth and rounded structure. The central region exhibits a bright, concentrated luminosity, potentially indicating a significant stellar population density or active galactic nucleus activity. Moving outwards from the core, the light intensity gradually diminishes, suggesting a decreasing stellar density with radial distance.

There is a hint of a diffuse, extended halo surrounding the central body, though it is faint and difficult to discern with certainty. No distinct spiral arms or bar-like features are readily apparent, leading to the preliminary conclusion that the galaxy may be elliptical or lenticular in morphology. There are no clear signs of any major tidal disturbances or ongoing mergers. The color is yellowish-orange.
