The galaxy appears to be undergoing a merger or interaction with at least one other galactic body. A larger, more prominent core exhibits a smooth, elliptical morphology, with a yellowish-white color indicative of an older stellar population. Extending from this core is a fainter, elongated tidal tail or arm-like structure, displaying a slightly redder hue, potentially due to dust extinction or a difference in stellar populations. The morphology of the system suggests that it could be an elliptical galaxy actively merging with smaller companion galaxies. There is evidence of morphological disturbance present in this object.
