The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits an elliptical or lenticular morphology, with minimal signs of spiral arms or distinct disk structures. The galaxy's light profile seems to gradually decrease in intensity from the core outwards, suggesting a lack of significant star formation in the outer regions. The object does not appear to be undergoing a major merger, though subtle disturbances could be present. The galaxy is more likely to be "in-between" in terms of roundness, rather than a perfect circle or a cigar-like shape. The galaxy appears generally undisturbed and somewhat evolved.
