The galaxy presents an overall smooth morphology, appearing as a slightly elongated spheroid. The central region exhibits a bright, concentrated nucleus, suggestive of a significant stellar density or possibly an active galactic nucleus. Moving outwards from the core, the galaxy displays a diffuse halo of decreasing brightness. Hints of a faint, flattened disk structure are barely visible extending along its major axis. The color gradient suggests older stellar populations dominate the core, while the fainter outer regions may contain younger stars and some star formation. There appear to be no prominent tidal features or signs of major mergers. The galaxy shows a intermediate roundness to its shape with no clear disturbances or interactions with other galaxies. Overall, the galaxy appears to be a relatively isolated system, potentially an early-type spiral or lenticular galaxy.
