The galaxy presents as a centrally concentrated object with a smooth overall morphology. There is little evidence of spiral arms or distinct features. The galaxy exhibits a radial color gradient, transitioning from a yellowish-white core to a more reddish outer region. The smooth light distribution suggests an elliptical morphology, with an approximate diameter of perhaps 4.5 kpc, give or take. Any ongoing star formation is likely minimal and mostly concentrated in the core of the object, with the outer portions of the galaxy appearing to consist of an older stellar population. No tidal tails or other signs of major interaction or recent merger activity are visible.
