The galaxy presents a largely smooth morphology, appearing elliptical in shape. A concentration of luminosity is observed at the galaxy's center, with the luminosity gradually diminishing towards the outer edges. The color profile is primarily redder, suggesting an older stellar population and a relative deficiency in active star formation. There is a slight hint of a disk-like structure, but it is very faint. There are no apparent signs of major disturbances due to mergers or tidal interactions with other galaxies in the vicinity.
