The galaxy presents as a moderately bright, disk-shaped object with an apparent size that is relatively small. Its color profile suggests a distribution of stellar populations, transitioning from a central, yellowish core to a more bluish outer disk. The core region exhibits a concentrated luminosity, potentially indicating an older stellar population or an active galactic nucleus, however it appears smooth. The bluer hues in the outer disk possibly indicate regions of active star formation. While the galaxy's overall structure is primarily smooth, some subtle distortions or irregularities are observable in the disk. There is an indication of possible minor tidal disturbance in the form of warping in one of the spiral arms, but this requires closer inspection to confirm.
