The galaxy presents as a somewhat compact object. The central region displays a notable brightness, possibly indicative of a concentrated stellar population or active galactic nucleus.

A ring-like structure surrounds this central brightness. The color is a mix, but with a reddish/pink hue, which may signify older stellar populations or dust obscuration within the ring.

Extending outward from the central region, a fainter, more diffuse halo or envelope is observed. This component appears more blue than red, perhaps suggesting a younger stellar population extending to the edge.

The overall form shows some asymmetry, potentially hinting at gravitational interaction or recent merger activity. Faint wisps or tidal features are suspected, requiring closer examination for confirmation. The light distribution indicates a slightly disturbed morphology rather than a purely elliptical or spiral structure.
