The galaxy presents as a somewhat elliptical, though mostly smooth object. It appears to have a concentrated central bulge, that gradually fades out into a diffuse halo. There is a slight asymmetry and what could be a disturbed morphology, but these are likely the result of either imaging artifacts or a minor gravitational interaction.

The galaxy's color appears to be dominated by older stellar populations, as evidenced by the red and yellow hues throughout. There are hints of bluer light, possibly indicating the presence of some younger stars, especially in a faint disk-like structure. Star formation is quite low. The overall impression is of a galaxy that has largely exhausted its gas supply and is transitioning towards a passively evolving system. The galaxy does not appear to be a strong merger candidate.
