The galaxy presents as a face-on spiral, exhibiting a moderately bright central bulge. Spiral arms are clearly visible, extending outwards from the bulge, and are relatively well-defined. The arms appear somewhat patchy, suggesting ongoing star formation within them. A bar structure seems to be present across the nucleus of the galaxy. There's no obvious sign of tidal disruption or interaction with other galaxies. The galaxy appears to be relatively isolated in the field. The overall color suggests a mix of stellar populations, with some regions showing bluer tints associated with younger, hotter stars, especially in the spiral arms, and the central bulge presenting a slightly redder, older population. The galaxy doesn't appear to be actively merging with any other discernible object.
