The galaxy presents as a generally smooth, elongated structure. Its morphology is seemingly that of a flattened spheroid, possibly an elliptical galaxy viewed at an oblique angle. The color profile suggests a prominence of older stellar populations, appearing reddish-yellow. There is no obvious spiral arm structure or dust lane obscuration, consistent with a lack of ongoing, significant star formation. The galaxy shows minimal signs of tidal disturbances or mergers. It appears fairly isolated in the field, showing no signs of interaction with nearby galaxies or objects.
