The galaxy appears as a central, concentrated bulge of light. It exhibits a yellowish hue, suggesting an older stellar population, and a red shift of approximately 0.26. The light appears fairly smooth and the image is fairly consistent with a general elliptical shape. While it appears mostly undisturbed, a small fraction of its morphology contains visual evidence of minor interaction or disturbance, likely due to a smaller merger in the past. The galaxy has an estimated mass of approximately 10^10.6 solar masses and an estimated star formation rate of 10^1.5 solar masses per year.
