The galaxy presents a relatively smooth, centrally concentrated luminosity profile, indicative of an elliptical or lenticular morphology. The light distribution appears mostly uniform, with a bright core that gradually decreases in intensity outwards. The galaxy exhibits a nearly circular shape, with a minor ellipticity observed. There is a slight color gradient from the center to the outer regions, with the core appearing whiter and the outer regions exhibiting a bluer hue. This suggests some level of ongoing or recent star formation in the outer regions of the galaxy. There are no distinct features such as spiral arms or a prominent dust lane visible. The galaxy appears undisturbed, without any signs of recent merger activity or tidal interactions.