The galaxy appears to be a relatively smooth, disk-shaped system, viewed at a moderate inclination. It exhibits a bright, concentrated central bulge that dominates the overall luminosity. The outer regions of the disk appear fainter and more diffuse, with no obvious spiral arm structure visible. There may be a very subtle indication of a dust lane present along the major axis. The overall color is indicative of a galaxy with a relatively older stellar population and a low rate of star formation. There is no apparent tidal features or signs of interaction.
