The galaxy presents as a somewhat elongated, cigar-shaped object. Its central region displays a concentration of light, possibly indicative of an aging stellar population, appearing more yellow in color. The outer regions of the galaxy exhibit a fainter, more diffuse blue hue. This may suggest ongoing or recent star formation within these areas, as younger, hotter stars tend to emit more blue light. The overall morphology suggests a galaxy which has undergone significant evolution. There is no obvious sign of a disk or spiral structure, and no signs of any major mergers or disturbances.
