The galaxy presents as an extended, diffuse object with a bright, somewhat amorphous central region. The overall shape appears elliptical, exhibiting a distinct flattening or elongation along one axis. Color gradients are evident, with the central region exhibiting a brighter, bluer hue that potentially indicates the presence of younger stellar populations.

The outer regions display a fainter, redder color, suggesting older stellar populations or dust obscuration. There are subtle, irregular features observable in the outer disk structure, possibly indicative of tidal interactions or past mergers, or simply uneven dust distribution.

Overall, the galaxy does not present a clear spiral structure and appears relatively smooth in morphology. There are indications of possible disturbances to its structure.
