The galaxy appears as a singular, luminous object with a smooth, elliptical morphology. It exhibits a dominant central bulge that appears nearly spherical. There is no evident spiral structure or prominent disk. The light profile suggests a concentrated distribution of stars, with luminosity decreasing steadily from the core outwards. The color of the galaxy is predominantly yellow-orange, possibly indicating an older stellar population and a relatively low rate of star formation. There are no significant signs of tidal interactions, mergers, or other morphological distortions. The galaxy appears to be largely undisturbed.
