The galaxy appears to be an elliptical galaxy, exhibiting a smooth, largely featureless morphology with a high degree of central concentration. Its shape is more akin to being in between round and cigar shaped, slightly elongated. There is no obvious evidence of spiral arms or a prominent disk structure. There may be evidence of a minor disturbance, with a slight distortion in its shape.

There is a noticeable color gradient within the galaxy, transitioning from more red in its core region to greener hues toward the outskirts. This suggests an older stellar population is centrally located, while younger, hotter stars may be present to some extent within the galaxy's outer regions. The redshift indicates that we are observing this galaxy at a significant distance from Earth.
