The galaxy presents an overall elliptical morphology, with a noticeable central bulge. The core region exhibits a high degree of luminosity, suggesting a concentration of stellar density and potentially an active galactic nucleus. Moving outwards from the core, the luminosity gradually decreases. The spiral arm structure is not clearly defined; the overall appearance is more akin to a smooth, relatively featureless spheroid. However, there appears to be some minor disturbance visible, a hint of asymmetry that could indicate gravitational interaction with a smaller galaxy. The outer regions of the galaxy have a faint extended halo of diffuse light. Some visual evidence of a minor merger or tidal interaction is suggested by faint asymmetries.
