The galaxy presents as an elliptical morphology, with a high degree of smoothness. It appears highly rounded. There is no evident disk or spiral structure discernable at this resolution, nor is there any evidence of tidal tails or strong gravitational disturbances indicating a recent major merger event. The galaxy exhibits a color profile that suggests a population dominated by older stars, with light distribution skewed toward the redder end of the spectrum. While the red shift may make this appear redder, it is intrinsically less blue than normal star forming galaxies at this red shift. Based on the overall magnitude and morphology, the galaxy is a relatively massive system and it is forming some stars, but not a large amount. There is no indication of an active galactic nucleus.
