The galaxy presents as a somewhat smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing more round than elongated. The core of the galaxy is bright and unresolved, likely indicating a dense stellar population or active galactic nucleus. Extending outward from the core, a diffuse halo of light is visible. The color of the galaxy is generally blueish-white, suggesting a moderate amount of recent or ongoing star formation. There may be some evidence of minor tidal disturbances or interactions, as slight asymmetry is seen in the extended halo. However, no major merging features or pronounced tidal tails are apparent. The overall structure points towards a spiral-like galaxy with a prominent bulge, however this may be disorted due to merger events.
