The galaxy presents a diffuse, somewhat amorphous morphology, indicating a system that may be undergoing significant gravitational interaction or a post-merger state. A notable lack of distinct spiral arms or a well-defined disk structure is observed. The light distribution appears relatively smooth, with a subtle central concentration. The galaxy's overall color is consistent with a slightly redder spectral energy distribution, potentially suggesting an older stellar population or the presence of significant dust obscuration within the system. Faint, asymmetric tidal features seem to extend from the main body, indicative of possible past or ongoing interactions with another galaxy. These features are more apparent on one side of the galaxy, which could be interpreted as evidence of an unevenly disrupted disk or a more recent merger event. No central bar structure or active galactic nucleus (AGN) is readily apparent in the image.
