The galaxy appears as a somewhat diffuse object, exhibiting a flattened, disk-like morphology. It is characterized by a generally smooth texture with only subtle variations in luminosity across its surface. Faint, disturbed features are visible, suggesting either a minor gravitational interaction or internal dynamics influencing its structure. While no well-defined spiral arms are discernible, the overall impression points towards a non-elliptical system. There is also evidence suggesting the galaxy might be undergoing a minor merger event or experiencing some form of disturbance. The light profile indicates a slightly reddish hue, and the object shows an intermediate size.
