The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is somewhat elliptical, appearing moderately rounded rather than highly elongated. There is little evidence of distinct spiral arm structures or significant dust lanes. The color profile suggests a dominant population of older stars, emitting a yellowish light, consistent with a redshift measurement indicating that the object is distant. The galaxy exhibits a relatively low star formation rate, given the general color, which indicates that the object likely ceased actively forming stars a significant time ago. There are no apparent major disturbances or merging events visible in the image, and the object appears relatively isolated. The overall morphology suggests the galaxy is likely an elliptical or lenticular type.
