The galaxy presents as an inclined spiral with a clearly defined disk structure. Its appearance is dominated by a moderate-sized bulge in the center, which exhibits a yellowish hue. The surrounding spiral arms display a bluer coloration, suggestive of ongoing star formation. While the arms themselves do not show extremely high-resolution detail, they can still be seen. The galaxy does not seem to be undergoing a major merger or strong tidal interaction, although a slight asymmetry can be observed in the disk, possibly indicating minor disturbances. The galaxy's elliptical shape suggests a relatively high inclination.