The galaxy appears to be an early-type spiral, potentially an Sa or Sb, exhibiting a prominent, bright central bulge. The bulge appears to be relatively smooth and featureless, suggesting an older stellar population. Fainter spiral arm structures are hinted at, exhibiting a blue hue which possibly indicates ongoing star formation within these regions, though they are not sharply defined and lack the resolution to discern distinct star-forming regions.

The overall shape of the galaxy is somewhat elongated, displaying an aspect ratio that is noticeably deviating from a perfect circle, tending toward an elongated shape. It is observed at an angle, not face-on. This makes it more difficult to clearly observe all morphological features. No indications of major tidal disturbances or interactions with other galaxies are apparent in the immediate vicinity. The galaxy presents an intermediate luminosity with a moderate size.
