The galaxy presents as a single, cohesive unit with a smooth, fairly uniform appearance, and is most likely an elliptical galaxy. The light distribution suggests a central concentration with a gradual fall-off in intensity towards the edges. The galaxy exhibits a warm hue, indicative of an older stellar population with lower levels of current star formation. The shape tends toward round. There is no apparent evidence of spiral arms, dust lanes, or strong tidal features; however, there is a possible merging object close to the galaxy. The galaxy appears well-formed, presenting a classical elliptical morphology at its estimated redshift.
