The galaxy presents a relatively smooth, elliptical morphology with a concentrated central bulge. The light distribution appears largely spheroidal, with no obvious spiral arm structure or distinct features. The color gradient suggests a possible stellar population gradient, with a yellow to reddish hue centrally and a slightly bluer tinge extending outwards. There is no strong indication of active star formation based on the smoothness of the light profile, the color, and lack of HII regions. It appears to be a galaxy at moderate redshift with the likely mass of a massive galaxy. 
