The galaxy appears as a relatively compact and centrally concentrated object. Its overall morphology seems smooth, with no readily discernible spiral arms or bar structures. The color profile suggests a mix of stellar populations, with a somewhat brighter, yellowish core, possibly indicating an older population of stars. The outer regions appear slightly bluer, indicative of some ongoing star formation. The galaxy exhibits a small angular size in the image, implying a considerable distance given its estimated luminosity. There are some subtle irregularities in its overall shape but it does not appear to have any major disturbances or indications of a recent merger event.
