The galaxy presents as a moderately bright, centrally concentrated object with a redshift indicating a significant distance. Its overall morphology appears relatively smooth, with a suggestion of a slight elongation. The light distribution seems fairly uniform across the galaxy's body, lacking prominent spiral arms or other distinct structural features. The color profile suggests a population of older stars, contributing to the overall reddish hue. There may be some minor irregularities in the outer regions, but these are not prominent enough to classify the galaxy as undergoing a major merger or disturbance. The galaxy appears to be relatively isolated in the image, with no obvious interacting companions immediately visible.
