The galaxy appears to be elliptical in shape, with a smooth, featureless morphology. The central region exhibits a bright, concentrated luminosity, suggesting a high stellar density. The color gradient transitions smoothly from a yellowish-white core to a dimmer, redder outer halo. There is no evidence of spiral arms, dust lanes, or ongoing star formation regions within the observable spectrum. The galaxy is relatively isolated, with no obvious signs of tidal interactions or ongoing mergers. The rounded shape indicates a relatively relaxed system, likely dynamically evolved.
