The galaxy presents a smooth, elliptical morphology, exhibiting a high degree of central concentration. Its overall color appears reddish, suggestive of an older stellar population dominated by evolved stars. There is a small but distinct companion galaxy nearby. There is little evidence of spiral arm structure or significant dust lanes. Given the observed characteristics, the galaxy is likely a relatively massive system with a low specific star formation rate. It is not experiencing any major mergers or disturbances. The galaxy is fairly round.