The galaxy appears to be a relatively compact, smooth object, likely an elliptical or lenticular galaxy. It exhibits a largely featureless profile with no apparent spiral arms or distinct structures. The galaxy presents a rounded morphology, displaying a high degree of symmetry. There is a hint of a very small disturbance, but overall it is a galaxy that has very little ongoing activity.

The object's color is dominated by a yellowish hue, which is indicative of an older stellar population, as well as a large quantity of dust and gas. No pronounced central bulge or visible nucleus is detected based on this image. The observed color suggests a possible suppression of recent star formation events.
