This galaxy presents as a flattened, disk-like structure oriented approximately horizontally in the image. The central region exhibits a higher surface brightness, suggesting a concentration of stars and possibly a bulge component. Progressing outwards from the core, the luminosity decreases gradually, with the edges appearing less defined and somewhat diffuse. The overall color is yellowish, indicating a population dominated by older stars, although subtle variations hint at some bluer regions potentially associated with younger stellar populations or ongoing star formation. There is no clear indication of a spiral arm structure or significant dust lanes from this view. Furthermore, there are no apparent signs of any major tidal disturbances or interactions with other galaxies. Based on its smooth appearance, it is either a relatively undisturbed late-type spiral galaxy or potentially an elliptical or lenticular galaxy seen edge-on.
