The galaxy presents as a somewhat elongated, elliptical structure. Its light profile appears smooth and centrally concentrated, exhibiting a gradual falloff in surface brightness from the core outwards. The dominant color appears to be a yellow-orange hue, suggesting a relatively old stellar population with fewer hot, young stars. No distinct spiral arms or prominent dust lanes are visible. There may be a slight indication of minor tidal disruption, but more data is needed to confirm this. The object's overall morphology suggests a galaxy that is not currently undergoing significant star formation.
