The galaxy presents a generally smooth, elliptical morphology, exhibiting a high degree of central concentration. The light distribution indicates an even profile from the inner region out to the edge, with no distinct features like spiral arms or bars. The overall shape is spheroidal, appearing highly rounded rather than elongated. The primary color component suggests an older stellar population dominated by redder wavelengths. Some bluer light may be present in the outskirts, potentially indicating some recent star formation. There is no indication of significant tidal disturbances or merger activity, and the galaxy does not appear to be interacting with any companion galaxies in the immediate vicinity.
