The galaxy appears as a concentrated, centrally brightened object, exhibiting a relatively smooth, elliptical morphology. The color profile suggests a population of older stars, with a yellow-red hue dominating the central region, indicating lower levels of ongoing star formation. There is a subtle greenish color gradient in the mid-section. The light is fading moving towards the outer regions. There is no obvious presence of spiral arms or a prominent disk structure. Based on its apparent structure, it is likely a massive galaxy. There is no evidence of significant tidal features or ongoing mergers.
