The galaxy presents as a fairly smooth and centrally concentrated structure. It appears as a flattened ellipsoid with a luminous, yellowish core, potentially indicating an older stellar population dominating the central region. Fainter, bluer light extends outwards from the core, suggesting the presence of some younger, star-forming regions within the disk. This disk displays a slight disturbance or asymmetry, possibly due to a minor interaction with another galaxy, although no obvious merging features are visible in this image. The galaxy exhibits a moderate redshift, indicating a substantial distance. Overall, the galaxy appears as a relatively massive system with an intermediate rate of star formation.
