The galaxy presents as a relatively compact structure with a dominant central region. The overall shape is somewhat irregular, showing features that could be indicative of gravitational interactions or ongoing mergers with other galaxies or galactic fragments. The core appears bright and diffuse, with an extended halo that fades into the background sky.

There are multiple distinct knots of concentrated light distributed throughout the galaxy, some with slightly bluer hues while others appear more reddish, possibly indicating regions of active star formation alongside older stellar populations. The galaxy does not exhibit a clear spiral or elliptical structure; it has a more amorphous appearance. There may be some tidal tails or disrupted features extending outwards, supporting a scenario of recent or ongoing gravitational interactions.
