The galaxy presents an overall elliptical morphology, showing a smooth light distribution without prominent spiral arms or a defined disk structure. The central region displays a concentrated luminosity, suggesting the presence of a galactic bulge. There is a slight elongation noticeable in its shape. The galaxy exhibits a redder color profile, potentially indicative of an older stellar population and/or significant dust content. Some faint features are visible, suggesting minor disturbances in the galaxy's structure possibly due to past interactions.
