The galaxy presents an overall elliptical morphology, appearing significantly elongated along its major axis. The light distribution is not perfectly smooth, with some subtle variations in color and brightness across the main body of the galaxy. A faint, diffuse halo surrounds the central region, extending further along the major axis. The core of the galaxy exhibits a relatively blue hue, suggesting the presence of younger stellar populations. There is an indication of potential disturbances or asymmetries within the galaxy's structure, such as a slight warping or tidal features. However, no major merger or significant interaction with another galaxy is immediately apparent. Some level of distortion is present, though the primary structure remains coherent.
