The galaxy presents a generally smooth, rounded morphology. There's a slight suggestion of a disk-like structure, but it appears dominated by a central bulge. The overall color is bluish-white, hinting at a population of younger, hotter stars, though it is possible that this may be a result of it's redshift. There is some irregularity, indicating a potential ongoing or recent interaction/merger, though signs of such are subtle. Given it's absolute magnitudes, the galaxy is not exceptionally luminous. Considering the color profile, a degree of ongoing star formation activity appears plausible.
