The galaxy appears to be elliptical in shape, with a smooth, diffuse light distribution and no immediately obvious spiral arm structures. The central region is brighter and denser than the outer regions. A faint tidal stream or extended feature may be present on one side of the galaxy, potentially indicating a past interaction or merger event, or evidence of a disk. The color appears to be shifted toward the blue end of the spectrum, which may indicate the presence of a population of younger, hotter stars.
