The galaxy presents as a relatively smooth, centrally concentrated object. Its overall color appears yellowish-orange, suggesting a stellar population dominated by older, redder stars with a diminished population of younger, blue stars. The morphology leans towards elliptical, appearing largely round in shape with no discernible spiral arm structure or significant disk component. There are no obvious signs of tidal disturbances or recent merger activity; the galaxy appears isolated and undisturbed. Its apparent angular size is small, indicating a substantial distance. The relatively uniform color distribution and lack of prominent features imply low ongoing star formation.
