The galaxy appears to be a relatively compact, elliptical galaxy. It exhibits a smooth, diffuse light distribution, with no clear spiral arm structures visible. The galaxy displays an overall yellowish-red hue, suggesting an older stellar population dominated by evolved stars. There is no evidence of significant dust lanes or active star formation regions within the visible portion of the galaxy. The morphology suggests that this galaxy may be undergoing little or no current star formation. The general shape appears close to round with only slight deviations. There is no obvious evidence of any major ongoing merger activity, although minor disturbances cannot be ruled out.
