The galaxy presents an ambiguous morphology, potentially indicative of a system undergoing interaction or exhibiting unusual internal structure. The light distribution within the galaxy is complex. A relatively bright, compact core appears present, though its exact morphology is difficult to ascertain given the image resolution. Emanating from this region is a fainter, more diffuse structure. This structure has a somewhat elongated appearance, perhaps suggestive of a tidal tail or disrupted arm. The color gradients within the galaxy show a slight variation. The core region appears bluer, indicating regions of recent or ongoing star formation, whereas the outer diffuse structure has a slightly redder color. The system is estimated to have an apparent diameter of ~3 arcseconds. Overall, the system demonstrates features indicative of either internal dynamical processes or external gravitational interactions that could be disrupting a disk galaxy. However, these interpretations need to be verified by spectroscopic or higher-resolution imaging.
