The galaxy presents as a smooth, elliptical morphology. It exhibits a cigar-like shape, noticeably elongated along its major axis. The light distribution is concentrated toward the center, suggesting a dense nucleus. The color gradient indicates a higher concentration of older stellar populations. There is no apparent evidence of spiral arms or significant dust lanes within the galaxy. There is no indication of active star formation from the visual data. Furthermore, there are no signs of tidal disturbances or ongoing mergers with other galaxies.
