The galaxy presents as a moderately luminous object, exhibiting an elongated morphology. A central, bright, and seemingly smooth component dominates the overall structure, suggesting a significant stellar bulge or nucleus. This central region displays a yellow-orange hue.

Extending from the central component is a fainter, more diffuse tail-like feature, which is also yellowish orange. This structure indicates a possible tidal interaction or disturbance. The morphology is broadly classified as intermediate in roundness, neither perfectly spherical nor highly elongated.

The galaxy's color suggests an older stellar population and relatively low star formation activity. Overall, the galaxy appears to be in a state of merging.
