The galaxy presents a generally smooth, elliptical morphology, appearing largely featureless upon initial inspection. Its light profile exhibits a centrally concentrated bulge that fades gradually into the outer regions. The core appears bright and yellowish, indicative of an older stellar population. A subtle color gradient is observed, transitioning to a slightly redder hue in the outer halo. There is no discernible evidence of spiral arm structure, dust lanes, or ongoing major mergers. Minor asymmetric disturbances cannot be ruled out, but the overall structure suggests a relaxed system that is evolving relatively peacefully. The galaxy is compact.
