The galaxy presents as a centrally concentrated system, appearing largely smooth in morphology. The light profile indicates a generally elliptical shape, showing only slight elongation. The color distribution appears relatively uniform, trending towards redder hues in the central region and slightly bluer tones in the outer regions, indicative of differing stellar populations. The absence of distinct spiral arms or a prominent central bar structure suggests a classification towards the elliptical or lenticular end of the Hubble sequence. There are no obvious signs of major mergers or tidal disturbances, though minor distortions can't be ruled out at this resolution. Overall, the galaxy appears to be a relatively massive system with moderate ongoing star formation activity.
