The galaxy presents an overall elliptical morphology, exhibiting a high degree of smoothness with a relatively featureless disk. The shape appears somewhat elongated, though not distinctly cigar-shaped, leaning towards a more intermediate form. The central region displays a higher concentration of light, indicating a possible bulge. The light distribution appears fairly symmetric. There is no visual evidence of strong tidal features or ongoing mergers, with the object appearing relatively undisturbed. The overall color profile appears slightly redder. This suggests a stellar population which is generally older. There is minimal evidence of ongoing star formation. 
