The galaxy presents as an elliptical morphology, appearing largely smooth and rounded in form. There is a concentration of yellowish light toward the galactic center, which could suggest an older stellar population. The outer regions exhibit a faint, diffuse halo with tinges of blue, which could indicate some ongoing, albeit low-level, star formation. No distinct spiral arms or significant dust lanes are discernible. There is potentially some slight distortion or minor disturbances in the galaxy's outer structure, but this feature is not highly pronounced. Overall, the galaxy appears to be a relatively quiescent system.
