The galaxy presents as a generally smooth, elliptical form, lacking any discernible spiral arm structure or prominent disk features. Its overall color appears yellowish, suggesting an older stellar population dominated by redder stars, and potentially lower levels of ongoing star formation. The galaxy's morphology is fairly regular, exhibiting a high degree of radial symmetry and little evidence of significant tidal disturbances or ongoing merger activity. It appears to be a relatively massive system, given its overall brightness and apparent size. There may be a faint extension or halo surrounding the brighter central region, though the resolution is insufficient to determine its exact nature. 
