The galaxy presents a smooth, elongated morphology. Its shape is more akin to a cigar than a perfect circle. The light is concentrated toward the center, suggesting a substantial bulge or core. The colour profile exhibits a clear gradient, shifting from a yellow-white core to a more reddish hue in the outer regions. This colour difference indicates that the outer portions could have a population of older, cooler stars while the core contains younger, hotter stars. Minor irregularities are present in its structure, perhaps implying a slight gravitational disturbance. Despite these minor features, the galaxy appears to be an isolated system. 
