The galaxy presents a mostly smooth appearance, with a concentrated central bulge. There is evidence of a disk structure, but it is not particularly prominent. The object exhibits a generally round morphology. Based on the color profile, there appears to be ongoing star formation, especially within the central region. The galaxy does not seem to be completely isolated, but rather shows signs of potential interaction or disturbance with its immediate environment. There is a possibility of a minor interaction or early-stage merger event. However, it should be noted that there is also a higher than expected artifact fraction. 
