The galaxy presents as a centrally concentrated object with a generally smooth appearance. The core exhibits a bright, intense central region. A faint disk-like structure surrounds the core. This structure appears slightly elongated.

There is some possible minor disturbance on the disk, but no clear signs of major mergers. The lack of defined spiral arms and the dominance of the central bulge suggest the galaxy is potentially of early-type morphology, possibly an elliptical or lenticular galaxy. The color gradient transitions from a bluer disk to a redder bulge.
