The galaxy presents as a blended spheroid, with a dominant, smooth central bulge and a partially resolved disk component. The overall morphology is consistent with an elliptical galaxy exhibiting characteristics of a recent or ongoing merger.

The core region is dominated by a bright, concentrated luminosity, indicating a high stellar density, likely composed of older stellar populations. Moving outward from the center, the light appears less concentrated. One side of the core is dominated by blue light, and the other side is dominated by red light. The disk-like structure shows signs of tidal disturbances, likely resulting from the gravitational interaction between the galaxy and a merging partner. Patches of distorted, irregular material extend from the main body, hinting at tidal tails or streams. These features lack a clearly defined spiral arm structure, suggesting a disruption to any prior organization within the disk.
