The galaxy appears as a concentrated, elliptical-shaped object with a smooth, featureless morphology. There is a high degree of central concentration of light, indicating a prominent bulge. The galaxy exhibits a general yellow-white color profile across its body, suggesting an older stellar population and lower levels of ongoing star formation. No dust lanes or spiral arm structures are obviously discernible. The galaxy does not appear to be undergoing any major merger activity or significant tidal disturbances. It presents as a relatively isolated system.
