The galaxy appears as a relatively small, faint object. The light profile suggests a somewhat compact nature. There is little indication of a prominent disk structure; the galaxy's light is distributed in a seemingly amorphous manner. A faint red hue permeates the galaxy, perhaps indicative of an older stellar population or significant dust obscuration. The overall morphology suggests the possibility of a recent or ongoing gravitational interaction or merger event. There is an irregular light distribution indicating disturbed morphology and tidal features such as streams. There is no clear central bulge, the light diffuses to the edges.
