The galaxy presents as a centrally concentrated structure with a bright, unresolved core, suggesting a significant stellar population in the nuclear region. The galaxy exhibits a somewhat irregular morphology, displaying features characteristic of a spiral galaxy, but lacks well-defined spiral arms. The overall color is moderately blue, which could indicate ongoing star formation, although the low estimated star formation rate indicates that this is minimal. There appears to be some evidence of dust lanes or irregular structures within the disk, potentially indicative of past or ongoing interactions. The galaxy does not display an obvious merging component, though minor disturbances or tidal features cannot be ruled out. The object has an apparent size that is relatively small, indicative of a galaxy at an intermediate distance.
