The galaxy appears as a somewhat diffuse, elliptical-like object with a relatively smooth profile. Its core is noticeably brighter and more concentrated than the outer regions. The galaxy exhibits a yellowish-red hue, which could suggest an older stellar population and a relatively low rate of on-going star formation. There is some indication of a disk-like structure, but no distinct spiral arms are apparent. There appear to be some minor disturbances to the galaxy, and the galaxy is most likely not currently undergoing a major merger. However, there may be a very small merger occurring.