The galaxy appears to be a lenticular or early-type spiral galaxy, characterized by a bright, centrally concentrated bulge. It exhibits a smooth, diffuse morphology with a faint disk component. The galaxy is not perfectly circular, displaying a slight elongation. There are no distinct spiral arms or prominent dust lanes visible, suggesting that recent or ongoing star formation is low. The overall color is relatively red, which is expected in older stellar populations with less star formation. No significant signs of interaction or recent merger activity are apparent.
