The galaxy presents a generally smooth morphology with a centrally concentrated luminosity profile. The object appears to be relatively round in shape, lacking any significant elongation or asymmetry. There is some evidence of faint, diffuse features or minor disturbances in the outer regions, but the dominant structure is a largely featureless core. The color gradient suggests a possible mixture of stellar populations, with the central region exhibiting a bluer hue compared to the slightly redder periphery. It is difficult to discern any spiral arms or distinct disk-like structures. A merger is unlikely. The galaxy may possibly be an elliptical galaxy. 
