The galaxy appears as a faint, slightly elongated structure with a moderate central concentration of light. Its overall color is a muted blue-white, suggesting the presence of a relatively old stellar population, but may also have ongoing star formation. There seems to be some slight irregularity in its shape, possibly indicating minor disturbances. There is no obvious presence of spiral arms or a well-defined disk structure. It is likely a galaxy with a mass toward the lower end. The overall faintness of the galaxy suggests a fairly low rate of star formation. The galaxy is not undergoing a major merger, however there may be signs of a minor disturbance event.
