The galaxy presents as a somewhat elliptical, face-on system. Its morphology appears to be largely smooth, suggesting a lack of prominent spiral arms or significant dust lanes. There is a central bulge, appearing slightly brighter and more concentrated. The color profile indicates a tendency toward bluer hues, which could imply ongoing, though potentially subdued, star formation activity within the galaxy. While no major disturbances are obvious, there is a slight asymmetry to the galaxy's outer regions, with faint hints of a possible interaction or minor disturbance.
