The galaxy appears to be a lenticular or early-type spiral galaxy, exhibiting a smooth, centrally concentrated luminosity profile. The light is yellowish-orange, suggestive of an older stellar population with relatively little ongoing star formation. The galaxy shows an elliptical shape, and the light becomes increasingly faint at its periphery. There is no evidence of spiral arms or dust lanes. There are hints of faint, diffuse light extending beyond the main body of the galaxy, potentially indicating a halo of older stars. Based on the color and morphology, it seems that the galaxy is a relatively massive system. No ongoing merger events are apparent, and the system appears largely undisturbed.
