The galaxy presents a spiral morphology, seen at a moderate inclination. Two distinct spiral arms are visible emanating from the central bulge. These arms exhibit a medium winding, suggesting an intermediate state between tightly wound and loosely defined spirals. The central bulge appears moderately sized. A bar structure is faintly discernible, with intermediate prominence. The disk is the dominant feature. There are no indications of any significant major mergers or disturbances in the galaxy's structure, though minor disturbances cannot be ruled out. Color gradients suggest a mix of stellar populations, with bluer regions indicative of recent star formation primarily along the spiral arms and a yellowish/redder central bulge suggesting a population of older, redder stars. The galaxy appears to be in a relatively isolated environment, with no immediate signs of interactions with other galaxies.
