This galaxy appears to be an elliptical or lenticular type, displaying a generally smooth and rounded morphology. It exhibits a centrally concentrated brightness profile, suggesting a prominent bulge component. Faint, diffuse features are visible, perhaps indicative of a weak disk or tidal disturbances but the smooth appearance would suggest this isn't the case. The color indices suggest a relatively old stellar population, dominating its light output. However, there is some bluer light that suggests there is potentially on-going star formation activity within the galaxy. There is no obvious spiral structure or bar feature. Based on its redshift, this galaxy is at a considerable cosmological distance. There may be an interacting companion or tidal debris present but without higher resolution or better color data, it is difficult to assess.
