The galaxy appears as a relatively small, faint, and somewhat elongated object. Its color is slightly bluish, suggesting the presence of a younger stellar population, though the overall color is not overwhelmingly blue. The galaxy does not present a strong spiral structure, but rather appears more amorphous and diffuse, with no clearly defined arms or central bulge. The luminosity of the galaxy appears moderate, typical of a dwarf galaxy. There is minimal evidence of active star formation. The smooth appearance suggests that it is likely an elliptical or lenticular galaxy, with a possibility that it is a disrupted spiral galaxy. There are no signs of on-going major mergers.
