The galaxy presents an overall elliptical morphology with a smooth, diffuse appearance. There is a prominent central bulge, appearing bright and concentrated in the visual band, that gradually fades into a surrounding halo. The outer regions of the galaxy are less well-defined, lacking a sharp boundary. No distinct spiral arm structures or prominent dust lanes are discernible. The color distribution suggests a predominantly older stellar population with a redder hue dominating the bulge and inner regions, with a slight blueing trend toward the outer parts, but still predominantly red. There appears to be low levels of recent or ongoing star formation. There is no strong evidence of any major ongoing merger event, although some minor disturbances may be present in the outer regions.
