The object presents as a galaxy with an apparent oblong morphology. The primary body of the galaxy exhibits a relatively smooth, though somewhat irregular, structure. Within the main body, two distinct, brighter central regions are observable, suggestive of either two galactic nuclei or areas of heightened star formation activity. The light distribution within these regions appears generally uniform.

Surrounding the brighter central regions is a fainter halo or disk component. This outer structure displays less distinct features than the central regions. There are hints of minor disturbances in the outer region, although the precise nature is difficult to assess from the image resolution. Some reddish patches or areas of lower blue wavelength emission can be seen primarily towards one side of the object, possibly indicative of dust obscuration or differing stellar populations.

Overall, the galaxy's appearance is suggestive of a system undergoing interaction or a recent merger, although the interaction does not appear to be a major disruption. The presence of the dual central concentrations contributes to this interpretation.
