The observed galaxy presents as a relatively small and faint object. The galaxy's morphology is difficult to definitively ascertain from this image. However, based on the visual impression and the additional information, there appears to be a faint, disk-like structure. There is also a suggestion of some morphological disturbance, potentially indicating a past or ongoing minor merger event. There appears to be a relatively smooth area towards one part of the galaxy, but no evidence of spiral arms. The galaxy shows a broad spectral energy distribution, with emission across green, red, and potentially Z bands.
