The galaxy presents an overall smooth morphology, appearing largely elliptical in shape with a high degree of circularity. There is a notable concentration of light toward the galactic center, suggesting a prominent bulge. The color profile indicates a redder hue, typical of galaxies dominated by older stellar populations. There's little evidence of distinct spiral arms or significant dust lanes. No signs of major mergers or tidal disturbances are readily apparent, although the presence of minor disturbances cannot be entirely ruled out at this resolution. Star formation seems to be suppressed based on its color. Overall, the galaxy seems to be a relatively massive, quiescent galaxy.
