The galaxy exhibits a disturbed morphology, potentially indicative of an ongoing or recent interaction. A prominent, elongated central bulge displays a smooth, yellowish-white color gradient, suggesting an older stellar population. Extending from this bulge is a fainter disk structure, exhibiting a clumpy appearance with hints of blueish regions. This could indicate areas of ongoing star formation, although the rate is likely subdued. One arm of the galaxy appears heavily disrupted, possibly due to gravitational forces. The overall shape deviates significantly from a regular spiral or elliptical form. A secondary, smaller object is visible, seemingly connected by a faint bridge of material, suggesting a possible tidal interaction or minor merger event. There is a moderate chance that this is not a true merger, but a more distant object.
