The galaxy presents a generally smooth morphology, lacking any prominent spiral arms or bar structures. The light distribution suggests it is an elliptical galaxy, although a faint disk cannot be ruled out based on this image alone. Its shape is approximately elliptical, displaying a slight elongation. There is no indication of any ongoing major mergers or significant tidal disturbances in the surrounding halo, although a slight asymmetry may be present, suggesting a potential minor interaction or recent accretion event. A faint blue tinge permeates the galaxy, particularly in the central region, hinting at the presence of at least some younger stellar populations and possibly ongoing, albeit low-level, star formation. The galaxy's integrated color appears somewhat bluer than typical elliptical galaxies, although much redder than a typical spiral galaxy.
