This galaxy presents as an elliptical morphology, exhibiting a smooth, concentrated light profile with a centrally dominant core. The object displays an apparent yellow-orange hue, suggestive of an older stellar population with a lower rate of ongoing star formation. The galaxy's shape is observed to be moderately elliptical, deviating from a perfectly circular form. No distinct spiral arm structures or dust lanes are discernible within the image, consistent with an early-type classification. There are no major signs of tidal disturbances or ongoing major mergers. The galaxy exhibits a relatively high level of smoothness, indicating that is a fairly relaxed stellar system. 
