The galaxy appears as a single, relatively smooth object with a central bulge. The galaxy exhibits a somewhat elongated morphology, but not strongly so, tending towards a more circular shape. The color profile suggests a redder hue, indicative of an older stellar population with suppressed levels of star formation. The smooth appearance and color are consistent with an elliptical galaxy, but further analysis is needed. There is no evidence of spiral arms or significant dust lanes visible in this image. There also appear to be no signs of any ongoing merging events. The galaxy seems to be undisturbed.
