The observed galaxy exhibits a structure characterized by both smooth and featured components. A bright, central bulge dominates the core region, displaying a relatively smooth texture. Moving outward from the bulge, a fainter, more diffuse disk structure becomes apparent. This disk reveals evidence of disturbances, possibly indicative of gravitational interactions.

The overall color profile suggests a mix of stellar populations, with a yellow-white hue prominent in the central bulge, potentially indicating older stars. The disk region displays some blue components, which could represent younger, hotter stars.

Significant disturbances appear present in the galaxy. There is significant disruption of the morphology, leading to apparent irregular features. Faint tidal tails or extended structures may be present, indicating a possible interaction with another galaxy.
