The galaxy exhibits a moderate redshift, suggesting it is at a considerable distance. Its morphology appears to be generally smooth, but not entirely featureless. There is a subtle indication of a disk-like structure or some internal features present within the overall smoothness. The shape is elongated, leaning towards a cigar-like form rather than being perfectly round. There are no obvious signs of a major ongoing merger, but some indications of a minor disturbance or interaction may be present. It exhibits a luminosity consistent with a galaxy of moderate mass and a corresponding star formation rate. The overall color profile suggests the presence of both older stellar populations and ongoing star formation.
