The galaxy presents as an elliptical morphology, appearing somewhat elongated or cigar-shaped. Its central region exhibits a bright, concentrated luminosity, suggesting a significant stellar population. Moving outwards from the core, the galaxy displays a gradual decrease in surface brightness. The color profile indicates a possible red-shift. Hints of disk features may be present within this galaxy's structure, however, the object is mainly smooth. No major disturbances or mergers are seen.
