The galaxy presents a face-on spiral structure. Spiral arms are apparent, exhibiting a somewhat patchy distribution of light, indicating regions of active star formation. The central bulge is clearly visible and appears moderately sized in comparison to the overall disk. Its color suggests an older stellar population. The galaxy's disk is the dominant feature, with the spiral arms extending outward from the central bulge. There is no sign of disturbance, however, the image quality limits our ability to identify any faint tidal features indicative of past or ongoing interactions.
