The galaxy presents as a slightly elongated, lenticular structure with a smooth, diffuse light distribution across the central region. There is a subtle colour gradient, with the core appearing marginally redder than the outer regions. This suggests an older stellar population concentrated towards the center. Faint wisps of bluer light are visible on one side of the disk, hinting at possible recent star formation regions. Overall, the galaxy exhibits a moderate redshift, indicating a significant distance. It appears relatively undisturbed, with no major signs of tidal interactions or mergers in progress, although some minor disturbances may be present. The absolute magnitude indicates that it is a fairly luminous galaxy. Its morphology is somewhere between elliptical and spiral with more elliptical qualities, possessing a large stellar mass. Its star formation rate is low, but is detectable.
