The galaxy presents a relatively smooth morphology, with a dominant, centrally concentrated light distribution. There is some indication of internal structure, but it appears mostly blurred. The galaxy appears slightly elongated, but mostly round. The color suggests the presence of both older stellar populations (redder hues) and some degree of ongoing or recent star formation activity (bluer/greenish hues). There is a potential merger or tidal interaction occurring, which is suggested by the presence of multiple less-concentrated regions of emission or some form of disturbance within the galaxy's overall structure. Overall, the galaxy appears to be a relatively massive system at moderate redshift, showing signs of interaction or a recent merger.
