The galaxy appears as a faint, elongated structure. The light is concentrated in the center, and a faint disc or spiral structure is present. There is an apparent irregularity to the galaxy's form, though it seems that it is not experiencing a major merging event. The galaxy's central bulge seems somewhat smooth, while the edges show some patchiness. The lack of more definitive structure could be a result of its distance. There may be some dust obscuring the galaxy. The color profile indicates a moderate degree of star formation and intermediate age stellar populations.
