The galaxy presents a generally smooth and rounded morphology. It exhibits a centrally concentrated light profile, appearing brightest at its core and gradually fading towards the edges. There are no prominent spiral arms or bar structures visible. The galaxy appears to be an elliptical galaxy.

The color of the galaxy is generally redder, suggesting a population of older stars. This is consistent with a lower ongoing star formation rate. There appears to be no major disturbance or interaction with other galaxies. The smooth, rounded shape and redder color indicate a galaxy dominated by an older stellar population, consistent with a well-evolved system.
