The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. Its overall form is elliptical, appearing mostly rounded with a subtle deviation toward an in-between shape rather than a perfectly circular or elongated one.

The galaxy's color profile indicates a prominent redder hue, suggesting an older stellar population with minimal ongoing star formation. The galaxy does not exhibit any obvious spiral arm structures or a prominent disk. No significant tidal tails, plumes, or distortions are readily apparent, indicative of a relatively undisturbed state, free of major ongoing mergers. There may be very minor disturbances.
