The galaxy presents an elliptical morphology, appearing cigar-shaped with a smooth and relatively featureless structure. Its core region exhibits a concentrated luminosity gradient, suggesting a high stellar density in the galactic nucleus. The color profile transitions from a central yellowish-white hue to a bluer periphery, indicating a potential variation in stellar populations and age distribution across the galactic body. There is no visual evidence of strong spiral arm structures or significant dust lane obscuration. Minimal signs of tidal disturbances or ongoing mergers are apparent. The galaxy appears to be an isolated system, undisturbed by major gravitational interactions with neighboring galaxies.
