The galaxy presents with an irregular morphology, lacking a clear spiral or elliptical structure. There is a brighter, compact core region exhibiting a bluish hue, potentially indicating ongoing star formation within that area. Surrounding this core is a more diffuse, fainter halo of light with a slight elongation in one direction, giving the galaxy an overall asymmetrical appearance. There are suggestions of minor disturbances in the distribution of light within the fainter halo region, such as the development of two fainter tails on the left side of the core region. These disturbances could be indicative of interactions or mergers with smaller galaxies. The central bulge is generally round but there are signs of minor disturbance and potential signs of merging features. Overall, the object appears to be a disturbed galaxy undergoing a minor interaction or merger.
