The galaxy appears to be a relatively smooth, lenticular or early-type spiral galaxy. It is elongated in shape, exhibiting an intermediate axial ratio. There is a subtle color gradient, with a slightly bluer hue present in the central region compared to the outer edges, suggesting some ongoing star formation. The overall luminosity indicates it is a substantial galaxy, consistent with a mass that is slightly higher than the Milky Way's mass. There is no obvious evidence of any major mergers or significant tidal disturbances in the image. Overall, it appears to be an ordinary field galaxy exhibiting normal evolutionary characteristics.
