The galaxy presents an elliptical morphology, appearing mostly smooth in texture with a concentrated central bulge. While a defined disk structure is not apparent, there appears to be some degree of asymmetry. The galaxy exhibits a yellowish hue, indicating a stellar population that is likely dominated by older, redder stars, suggesting a relatively low star formation rate. There is a slight visual disturbance in the form of faint arms or tidal tails that could suggest a minor interaction or recent merger event. This galaxy is relatively compact.