The galaxy exhibits a complex morphology. It appears to consist of at least two distinct components. A central, bright, roughly spherical region of bluish-white color dominates the core. This possibly indicates a concentration of young, hot stars, potentially within a bulge or core component.

Extending from this central region is a fainter, more diffuse structure with an elongated morphology. This extension displays a yellowish-red hue, suggesting an older stellar population with lower temperatures or dust obscuration. There is a hint of a disk-like feature, but it appears disrupted or irregular, with some indications of tidal tails or asymmetric features. The overall structure appears moderately disturbed, which could indicate a merger or interaction with another galaxy. Further analysis is required to fully understand the nature and history of this object.
