This galaxy exhibits an elliptical morphology, appearing elongated and cigar-shaped. The core of the galaxy presents a bright, concentrated luminosity, which gradually decreases outward. The light distribution suggests a relatively smooth, featureless structure, with no discernible spiral arms or prominent dust lanes visible in this image. The galaxy possesses a redder hue in comparison to spiral galaxies which indicates an older stellar population, with possible ongoing low-level star formation. The outer regions display a fainter, diffuse glow, transitioning smoothly into the background sky. There are no obvious signs of tidal disturbances or interactions with other galaxies.
