The galaxy presents a smooth, elliptical morphology. The light distribution appears centrally concentrated, with a gradual decrease in intensity outwards. A slight elongation is observed in the galaxy's shape, creating a flattened appearance, though not strongly so. The overall color profile suggests a predominantly older stellar population, with a yellowish hue, implying a lack of significant recent star formation activity within the main body of the galaxy. There appears to be minimal evidence of spiral arm structures, with some subtle irregularities on one side.
