The galaxy presents as a lenticular or early-type spiral galaxy, exhibiting a prominent bulge with a smooth, elliptical light distribution. The core is bright and concentrated, transitioning smoothly into a less luminous, extended halo or disk. There is a subtle flattening of the galaxy suggesting that it is not completely spherical. I am able to vaguely see a hint of possible arm structure, though it is tightly wound, faint, and difficult to resolve given image quality. The color gradient indicates a higher concentration of older stars in the central bulge, which transitions to slightly bluer and more complex populations in the outer regions. There is no obvious ongoing star formation, but rather a low and gradually declining rate. I do not see any clear signs of a recent merger event or major disturbance, although there might be some fainter components which could point to this.