The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer edges. The galaxy's overall shape is generally round, with only slight deviations from perfect circularity. There is no prominent disk structure visible, nor are any distinct spiral arms apparent. The light distribution appears fairly uniform, suggesting a lack of significant ongoing star formation or major dust lanes. Based on the limited details discernible, the galaxy appears undisturbed with no signs of ongoing or recent merger activity. The galaxy has an apparent color index which corresponds with galaxies with older stars and less active star formation.
