The galaxy presents as a relatively smooth, centrally concentrated system, exhibiting an elliptical morphology. There is a subtle elongation of the galaxy, indicating a deviation from a perfectly circular shape. The color profile suggests a redder central region transitioning to bluer outer regions. The galaxy lacks any discernible spiral arms or prominent dust lanes. There is no obvious indication of a recent major merger. The overall appearance of the galaxy suggests a mature stellar population with ongoing, but not vigorous, star formation in the outer regions.
