The galaxy presents as a disk galaxy, viewed at an inclined angle. A prominent central bulge is observed with a yellow-orange hue, suggesting an older stellar population and reduced star formation activity within this region. The disk component is significantly larger than the bulge, exhibiting a bluer color gradient towards the outer regions, indicative of younger stars and ongoing star formation. Tightly wound spiral arms emanate from the central bulge, displaying a flocculent structure with distinct regions of star formation evidenced by the presence of bright, blue knots distributed along the arms. These spiral arms are not sharply defined, appearing somewhat fuzzy and intermixed. The overall morphology suggests a disk-dominated spiral galaxy, with a moderate degree of inclination relative to the observer's line of sight. There are no obvious signs of a major ongoing merger, though some minor irregularities in the spiral arm structure could suggest tidal interactions or disturbances. The galaxy appears relatively isolated in the observed field.
