The galaxy presents as a primarily smooth structure, with a hint of disk-like morphology. The central region exhibits a concentrated luminosity with an orange hue, suggesting an older stellar population and possibly a moderate level of dust obscuration. The outer regions show a slight elongation, deviating from a perfectly circular shape. There is a subtle blue tinge on the outer edges which could indicate a small amount of star formation. A slight asymmetry or minor disturbance is visible to one side of the main body which could indicate a possible ongoing interaction or past merger event.
