The galaxy appears to be a lenticular or an edge-on spiral galaxy, exhibiting a smooth, elongated profile. The central bulge is prominent and appears yellowish, suggesting an older stellar population. A faint, flattened disk is visible extending outwards from the bulge. The disk exhibits a subtle blueish hue towards its outer edges, hinting at the presence of younger, hotter stars within the galaxy. There are no clear signs of spiral arm structure visible, nor are there any indications of active galactic nuclei activity. No prominent dust lanes are observed. Overall, the galaxy appears to be a relatively undisturbed system.
