The galaxy appears as a centrally concentrated object with a smooth, relatively featureless morphology. The light profile suggests a single dominant component rather than a resolved disk or spiral arms. There is an apparent slight elongation, but it's largely circular. There is a central concentration of bright light, indicating the possible presence of an actively star-forming central region or an active galactic nucleus. The overall color is slightly bluer, suggesting the presence of a population of younger, hotter stars, indicating ongoing star formation. The galaxy does not show any signs of major mergers or significant tidal disturbances. The structure appears undisturbed and regular.
