The galaxy presents a relatively smooth, elliptical morphology, characterized by a high degree of central concentration. The light distribution appears fairly uniform across the main body, with a gradual decrease in intensity from the core outwards. The galaxy exhibits a yellowish-red hue, suggesting an older stellar population and relatively low ongoing star formation activity. There is a lack of discernible spiral arms or prominent features. The overall shape is generally round, with only minor deviations from perfect circularity. No signs of major mergers or tidal disturbances are apparent.
