The galaxy appears to be a relatively small, faint object with an estimated effective radius suggesting compact dimensions. It has a generally smooth morphology, with the majority of citizen scientists identifying it as smooth. There are no signs of a prominent disk structure, but a hint of a central bulge can be seen.

A slight disturbance in the shape is observed, as is also noted in the observations suggesting possible minor gravitational interaction with another galaxy or tidal effects. There are no other indications of major mergers or strong tidal features, as there is a consensus that the galaxy is not involved in an ongoing major merger.
