The galaxy presents as a diffuse, irregular object with a generally bluish hue. The light distribution suggests a structure undergoing significant gravitational disturbance. There appears to be a central, slightly brighter region with an extended, less concentrated arm or tail-like feature emanating from it. This feature exhibits a clumpy morphology, possibly indicating regions of enhanced star formation or tidal debris. Overall, the galaxy's shape is highly asymmetrical, hinting at a possible recent or ongoing merger event or tidal interaction with another galaxy. The galaxy exhibits weak overall luminosity, inferring it is a smaller galaxy.
