The galaxy exhibits a prominent, roughly spherical central bulge, characterized by a yellowish-white color. Surrounding the bulge is a fainter, more diffuse halo extending outwards.

A distinct feature is a ring-like structure surrounding the central bulge. This ring appears clumpy, with regions of enhanced blue emission, possibly indicating areas of active star formation. The ring appears asymmetrical.

There is evidence of tidal tails or streams extending outwards from the main body of the galaxy. These tails are bluer in color, suggesting a population of younger stars and/or ongoing star formation.

Overall, the galaxy displays signs of a possible ongoing or recent interaction or merger, evidenced by the ring and tidal tails, which have likely disrupted the galaxy's morphology.
