The galaxy presents as a diffuse, reddish-orange object with a seemingly irregular morphology. There is an indication of multiple bright knots of light, suggesting either distinct star-forming regions, the remnant nuclei of smaller galaxies interacting with the main body, or simply regions of higher stellar density within a single, distorted structure. The overall shape lacks a clear spiral or elliptical form, implying that it may be the result of a merger event, or a dynamically young galaxy that has not yet settled into a regular morphology. The lack of clear features makes it difficult to assess its stage of evolutionary development, other than that it has a significant red-shifted value that suggests it is at a considerable cosmological distance. The redder color suggests that its light is dominated by older stars and/or obscured by dust.
