The galaxy presents as a spiral type, characterized by prominent, well-defined spiral arms extending from a central bulge. Two spiral arms can be clearly distinguished, exhibiting a moderately wound morphology. The central bulge appears relatively bright and diffuse, indicating a moderate concentration of stars. The disk of the galaxy appears inclined with respect to our line of sight, but not quite edge-on. Some regions of the spiral arms appear bluer in color, potentially indicative of ongoing star formation within these regions. The overall structure exhibits some irregularities, which may suggest minor gravitational interactions or disturbances. There is no clear evidence of a major ongoing merger, although subtle asymmetries are present.
