The galaxy presents a somewhat elliptical morphology, though some disk-like features are suspected. The light is concentrated toward the center, suggesting a prominent bulge. The light profile appears fairly smooth. A faint extension is suggested at the edges. Hints of blue color are visible, which suggests a higher rate of star formation compared to galaxies with primarily older, redder stellar populations. Based on the appearance, a recent interaction or merger is possible, and the star formation rate could be elevated from such an interaction. This galaxy's mass is likely between 10^9 and 10^10 solar masses.
