The galaxy presents as an elliptical morphology, exhibiting a smooth and concentrated light profile. There is a high degree of central concentration, with the luminosity decreasing gradually outwards from the nucleus. The color profile is indicative of an older stellar population, showing a redder hue centrally that shifts to a yellow-red gradient towards the outskirts. There is little evidence of spiral arms or active star formation. The galaxy has a cigar shape, with no significant signs of tidal disturbances or ongoing mergers. The appearance suggests a relaxed system, likely a giant elliptical galaxy that has undergone significant evolution and quenching of star formation.
