The galaxy presents a generally smooth morphology. It exhibits an elliptical shape, appearing elongated rather than perfectly circular. The central region displays a concentrated, bright core that diffuses outward. Coloration indicates a likely older stellar population, with a yellowish-orange hue dominating. There is little to no evidence of prominent spiral arms or distinct dust lanes. Subtle color gradients suggest a variation in stellar population or metallicity from the core to the outer regions. The galaxy appears to be isolated, with no obvious signs of tidal interactions or ongoing mergers.
