The galaxy presents as a relatively smooth and elliptical-like structure. Its color profile appears to be dominated by redder hues, suggesting an older stellar population with diminished recent star formation. The galaxy exhibits a centrally concentrated luminosity profile, with the light intensity decreasing gradually towards the outer regions. There is no clear indication of spiral arms or significant dust lanes. No strong signs of tidal disturbances or ongoing mergers are apparent in the image. The overall morphology suggests an evolved galaxy, possibly a giant elliptical, residing at a considerable distance.
