The galaxy appears to be a relatively smooth, elliptical type. It exhibits a central bulge that appears luminous and concentrated, with a yellowish hue. The galaxy seems generally rounded, although not perfectly circular. There is little evidence of spiral arms or a well-defined disk structure. No significant tidal features or other major disturbances are apparent, suggesting a relative lack of recent merger activity. The color profile suggests an older stellar population, with little evidence of ongoing, high-rate star formation.
