The galaxy presents a complex morphology, exhibiting characteristics that suggest both smooth and potentially disturbed features. The primary structure appears elliptical, with a bright, concentrated core indicative of a significant bulge component. A distinct, flattened disk-like structure seems to surround the bulge, displaying a yellowish hue, possibly indicating an older stellar population. 

There's evidence of possible tidal features or minor disturbances, with faint extensions of light emanating from the main body. A brighter, bluish region is observed in the upper section, indicative of potential star formation or a region dominated by younger, hotter stars. However, the overall appearance is relatively smooth, not displaying strong evidence of major mergers or significant ongoing starburst activity across the whole galaxy. The galaxy has a redshift of approximately 0.2, placing it at a considerable distance.
