The galaxy exhibits a roughly elliptical morphology with a bright, concentrated core region. The core displays a predominantly blue hue, suggesting the presence of younger, hotter stars and ongoing star formation activity. Surrounding the core, there is a less luminous, more diffuse disk. The disk displays variations in color, transitioning from blue to redder tones moving away from the core which may be due to older stellar populations and dust obscuration in the outer regions. Subtle irregularities are observed in the disk structure, potentially indicative of minor gravitational disturbances, possibly hinting at a past or ongoing merger event. The overall color distribution implies a non-uniform stellar population, with the core being dominated by younger stars and the disk harboring a mix of younger and older stars.
