The galaxy presents as a generally smooth, elliptical morphology. The central region exhibits a high degree of luminosity, appearing nearly circular. The isophotes gradually decrease in intensity moving outwards from the core, maintaining an overall rounded shape. There is minimal visible substructure or indications of spiral arms. The galaxy's color appears generally yellow/red, suggesting an older stellar population with a relatively low rate of recent star formation. There is little to no evidence of ongoing merger activity or significant tidal disturbances in the immediate vicinity.
