The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, featureless morphology with a central bulge that appears relatively prominent. The light distribution suggests a high degree of radial symmetry with minimal or no spiral arm structure visible. The color profile suggests a dominant population of older stars, indicated by a yellow to reddish hue, particularly concentrated in the bulge. There's no noticeable dust lane obscuring the galaxy's center. There's a lack of bright blue or white regions, implying a low rate of recent or ongoing star formation. The outer regions of the galaxy fade gradually into the background sky, without any distinct tidal features or interactions.
