The galaxy presents as a somewhat compact object with a generally circular morphology. The light distribution suggests a centrally concentrated structure, though it is not perfectly symmetrical. The dominant color is a bright bluish-white, possibly indicating the presence of a younger stellar population and ongoing star formation in the central regions. A fainter, more diffuse reddish component is visible to one side, potentially representing an older stellar population or dust obscuration. There are indications of some disturbance or interaction, possibly a minor tidal feature, affecting the overall shape and light distribution. The galaxy does not present with tightly wound spiral arms or a bar.
