The galaxy presents as a relatively smooth, centrally concentrated object. It appears as a lenticular or early-type spiral galaxy, where the spiral arms, if present, are tightly wound and difficult to distinguish from the bulge. The central region exhibits a brighter, yellowish hue, suggesting an older stellar population. Moving outward from the core, the color transitions towards a slightly bluer shade, hinting at the presence of younger stars. The morphology is generally elliptical in projection. There is a hint of a faint, slightly disturbed disk-like structure, possibly caused by minor interactions. Overall, the galaxy appears relatively quiescent with a low star formation rate.
