The galaxy presents as a spiral system, exhibiting a face-on orientation relative to our line of sight. Its structure is characterized by a central bulge, from which spiral arms emanate. These arms are not highly defined, displaying a somewhat flocculent morphology. The color profile suggests a mixed stellar population, with a bluish tint indicating ongoing star formation concentrated within the spiral arms, while the bulge appears more yellow, suggesting a population of older stars. The galaxy exhibits a moderate degree of symmetry, with no obvious signs of major tidal disruption or ongoing mergers. There are some hints of potential minor disturbances, but there are no distinct features suggesting strong interactions. The galaxy possesses a moderate apparent size.
