The galaxy presents as a spiral type, displaying a prominent disk structure. Spiral arms are discernible, exhibiting a tightly wound morphology. There appears to be a moderate bulge present. Star formation is indicated, based on the luminosity and color of the spiral arms, though the overall star formation rate appears relatively low. There is a possibility of tidal distortion within the galaxy itself. The galaxy's stellar mass falls within a range appropriate for the observed luminosity and star formation rate.
