The galaxy presents as a centrally concentrated object with a moderately smooth overall appearance. Its shape is somewhat elliptical, leaning towards an intermediate roundness rather than a perfect sphere or a highly elongated form. There is a suggestion of disturbance in the morphology, possibly indicating a past or ongoing interaction, though not a major disruptive event. Redder hues are seen towards the center, potentially indicative of an older stellar population or dust obscuration, while a slightly bluer color is seen within the main disk, suggesting ongoing star formation activity. The galaxy's estimated size is considerable, which, coupled with the observable colors, may imply a sizable, actively evolving system at the observed redshift.
