The galaxy presents as a lenticular or early-type spiral, with a notable central bulge that appears relatively smooth and bright. The disk component is subtly visible, exhibiting a flattened elliptical shape with a high degree of axial symmetry, and some apparent elongation. The color distribution suggests an older stellar population, with a dominance of redder hues indicative of evolved stars and potentially lower levels of ongoing star formation. There is no clear indication of prominent spiral arm structures or significant dust lanes. The galaxy's morphology appears undisturbed, suggesting it has not undergone any recent major interactions or mergers. Overall, it presents a quiescent appearance.
