The galaxy presents with a mostly smooth morphology and a round shape. There is little evidence of defined spiral arms or a central bar structure. The light distribution suggests a concentrated central bulge that transitions to a more diffuse outer region. 

The color gradient indicates a general shift from bluer wavelengths in the outer regions to redder wavelengths in the center. This may indicate older stellar populations are concentrated in the galaxy's core with star formation potentially occurring in the outer areas. The presence of a slight asymmetry, or minor disturbance, in the galaxy's morphology could possibly indicate an ongoing or recent interaction with another galaxy, despite a general appearance suggesting it is not currently undergoing a major merger.
