The galaxy appears to be a relatively smooth, elliptical galaxy, approximately circular in shape. There is a central, bright bulge that fades gradually into the outer regions. No distinct spiral arms or disk-like structures are apparent. The overall color of the galaxy is a pale blue-white, suggesting the presence of a moderate population of young, hot stars, or relatively recent star formation, though the dominant morphology points to an older stellar population overall. There is no evidence of any significant ongoing mergers or major disturbances affecting the galaxy's structure. A very minor irregularity or possible tidal feature might be present on the periphery of the galaxy, however it is unclear. The galaxy appears fairly isolated.
