This galaxy appears to be a relatively smooth, elliptical system. The central bulge exhibits a yellowish hue, suggesting an older stellar population. The galaxy appears moderately elongated with a slight cigar shape. There is little evidence of spiral arm structure or significant dust lanes. A weak disk component may be present. There are no obvious signs of a major ongoing merger, though some minor disturbances cannot be ruled out. The red shift of the galaxy indicates that it is a distant object. The color profile and morphology suggest a galaxy with moderate mass and subdued star formation.
