The galaxy presents as a spiral type, oriented approximately face-on to our line of sight. It exhibits a distinct disk structure with spiral arms visible, though moderately flocculent. The spiral arms display a winding pattern. The central bulge is present and appears relatively small compared to the overall disk size. The luminosity profile suggests a moderate mass and a rate of star formation that is fairly low. There is some visual asymmetry, with some areas of distortion, which could be due to a minor interaction, as I do not observe an obvious merger event. A faint bar is suspected in the central region. The color of the galaxy appears bluer throughout the disk, with some hint of redder hues towards the central bulge.
