The galaxy presents as an elongated, elliptical structure. Its central region exhibits a concentrated, yellowish hue, suggesting a population of older stars. Moving outward from the core, the color gradient shifts towards bluer tones, hinting at the presence of younger stellar populations and possibly ongoing star formation within the galaxy's outer regions. The overall morphology appears relatively smooth, with no obvious signs of spiral arms or a prominent disk structure. There is a subtle irregularity observed along the galaxy's periphery, potentially indicative of minor gravitational interactions or past merger events. The galaxy exhibits a substantial size, indicating that it could be a massive galaxy.
