The galaxy presents as a somewhat elongated object, with a noticeable concentration of light toward its center. The central region exhibits a yellowish-orange hue, suggesting an older stellar population. Fainter, bluer regions are visible at the top and bottom parts of the galaxy. Based on the irregular shape and distinct features, this object appears to be the result of a merger or close interaction between two or more galaxies. The lack of well-defined spiral arms or a smooth elliptical profile supports this hypothesis. There is some indication of tidal tails emanating from the galaxy, which are often indicative of gravitational disturbance. The brighter central region may represent the combined nuclei of the merging galaxies.