The galaxy appears to be an elliptical morphology, exhibiting a generally smooth light distribution without readily apparent spiral arms or a well-defined disk structure. The central region is characterized by a high concentration of light, appearing bright and somewhat orange-red in color, suggestive of an older stellar population. Fainter, more diffuse light extends outwards from the core, displaying a gradient towards bluer hues in the outer regions of the galaxy. There are no obvious signs of recent major merger events. There might be some minor disturbances in the outer halo, but not enough to suggest that this galaxy is a merger.
