The galaxy presents a flattened, elongated morphology suggestive of a lenticular or edge-on spiral galaxy. A prominent central bulge exhibits a yellowish hue, possibly indicating an older stellar population with diminished ongoing star formation. Extending outwards from the bulge, a fainter, bluer disc is observed, though details of spiral arm structure are not readily discernible from the image. The disc's color suggests the presence of younger, hotter stars, though the smoothness of the disc implies that star formation rate is moderate. Overall, the galaxy appears relatively undisturbed, without strong evidence of recent major merger events or significant tidal interactions. The smooth appearance, intermediate colors, and lack of prominent features suggests an intermediate classification between elliptical and spiral galaxies.
