The galaxy appears as an asymmetric, moderately bright object. Its morphology suggests characteristics of both a smooth elliptical galaxy and a galaxy with a disk component. There is a central bright region that fades toward the edges. The galaxy exhibits an intermediate level of roundness, not perfectly spherical but also not highly elongated. There appears to be some minor disturbance to the galaxy's structure which could indicate an ongoing interaction or past merger event. The galaxy possesses a significant rate of star formation. Based on its color indices, it displays relatively strong emission across the green, red, and z bands.
