The galaxy presents as an elliptical or lenticular type, characterized by a relatively smooth, featureless morphology. There is a subtle concentration of luminosity towards the galactic center. The overall shape appears more rounded than elongated, with no discernible spiral arm structure or significant dust lanes visible. The galaxy exhibits a color profile suggestive of an older stellar population, trending towards the redder end of the spectrum. There is no immediately apparent evidence of ongoing major merger activity or significant tidal disturbances. 
