The galaxy presents as a largely smooth, elliptical structure with a concentrated central bulge that exhibits a warm, yellowish hue, indicative of an older stellar population. The surrounding halo displays a more diffuse and variegated color palette, transitioning into cooler blue and green tones. These cooler tones suggest the presence of pockets of younger stars and potentially ongoing, albeit low-level, star formation. Overall, the galaxy demonstrates a high degree of rotational symmetry, lacking any major signs of recent merger activity or significant tidal distortions. The galaxy appears to be relatively isolated in its environment.