The galaxy presents as a single, relatively smooth object with a slight asymmetry. It exhibits an elongated shape, deviating from a perfectly circular morphology. The core region is moderately concentrated. There is a hint of disturbance in the structure. The galaxy has an estimated effective radius of approximately 5 kpc. It has a stellar mass on the order of 10^11 solar masses and a relatively low star formation rate. The color suggests a redder population of stars.
