The galaxy presents as a relatively smooth, concentrated structure. Its morphology is generally elliptical, with a gradual increase in luminosity towards a bright, compact nucleus. The outer regions exhibit a more diffuse glow, indicative of a decreasing stellar density with increasing radius. The galaxy appears to be dominated by older stellar populations, given its overall color. There is no readily apparent dust lane, spiral arm structure, or other prominent features suggesting active star formation. The galaxy does not show signs of major tidal disturbances or interaction with other galaxies, though there may be a very subtle, minor asymmetry. 
