The galaxy presents as a relatively smooth, elliptical structure. There is a high degree of central concentration with a gradual decrease in luminosity towards the outer regions. There is little evidence of a disk or spiral arms. The overall color appears to be skewed toward the redder end of the spectrum, suggesting an older stellar population with lower rates of star formation. It appears fairly isolated with no obvious signs of ongoing mergers or major tidal disturbances, though a hint of asymmetry suggests possible minor interaction. The galaxy exhibits a generally round morphology.
