The galaxy presents as a centrally concentrated object with a generally smooth morphology. It displays an elliptical shape, appearing somewhat elongated but not significantly so. A dominant, bright central bulge is evident, with light gradually decreasing outwards. No distinct spiral arms or bar structures are apparent, suggesting a lack of significant disk component. The galaxy exhibits a reddish hue, indicative of an older stellar population and potentially significant dust content. There is only slight evidence of any ongoing or recent major merging events based on its overall structure. There is some subtle blueness noticeable in the outer regions of the galaxy which may indicate a small amount of star formation.
