The galaxy presents as a somewhat diffuse object, elongated in shape. It exhibits a relatively smooth texture, although there are hints of subtle structural variations within. A slight concentration of luminosity is observed towards what may be its center, but a distinct, well-defined core is absent. The color profile appears relatively uniform across the galaxy's extent, suggesting a consistent stellar population or dust content. There may be some very slight asymmetry in the outer regions, though it is hard to confirm given the image quality. There is nothing to strongly suggest that the galaxy is undergoing a major merger, but there is a suggestion of a minor disturbance. There are no obvious spiral arms or prominent features.
