The galaxy appears as a moderately luminous object with a relatively smooth morphology. Its overall form is somewhat elliptical but shows irregularities, suggesting potential interactions or internal disturbances. Color gradients are present within the galaxy, with a central region exhibiting a yellowish hue, potentially indicative of an older stellar population. The outer regions appear bluer, possibly due to ongoing star formation. There is faint evidence of extended structures or tidal tails, suggesting possible merger activity with another galaxy. Based on its redshift, this is a fairly distant galaxy.
