The galaxy appears to be an elliptical galaxy with a pronounced cigar shape. It exhibits a smooth, featureless morphology. The color gradient indicates a concentration of older stellar populations, with a yellowish hue dominating the central region and transitioning to a redder shade further out, suggesting a diminished rate of star formation. There is no distinct nucleus, but rather a smooth increase in brightness towards the center. There is no clear evidence of a disk component, spiral arms, or ongoing major mergers. The overall light distribution suggests the galaxy is relaxed and mature.
