The galaxy presents as a lenticular or possibly early-type spiral with a subtle disk component. Its overall structure is characterized by a smooth, centrally concentrated light distribution, suggesting an older stellar population dominates the bulge. A slight flattening is observed, with the major axis oriented roughly northeast-southwest. The presence of bluer hues in certain regions, potentially along the galactic plane, hints at some ongoing star formation, although it is likely subdued. There's no obvious presence of prominent spiral arms or dust lanes that may obstruct observations. The galaxy seems to be in a relatively quiescent state, devoid of major merger signatures.
