The galaxy presents as a lenticular or early-type spiral, exhibiting a smooth, elliptical morphology with a high degree of central concentration. The light profile transitions gradually from a bright, yellowish core to fainter, reddish outer regions. There's no discernable spiral arm structure, indicating a predominantly bulge-dominated system. The lack of prominent dust lanes or bright, knotty regions suggests relatively low levels of current star formation. The highly elongated shape implies a significant degree of rotational support. Overall, this galaxy appears to be a relatively massive, evolved system with a substantial stellar population.
