The galaxy presents as a nearly elliptical, smooth object with a concentrated central bulge. Its overall color appears to be a bluish-white hue, suggesting the presence of a moderate population of younger, hotter stars. There is little evidence of spiral arm structure or significant dust lanes. The galaxy exhibits a relatively high degree of symmetry, with a gradual decrease in luminosity from the center outwards. No obvious signs of recent mergers or tidal disturbances are visible. The object appears to be relatively isolated, with no clear interactions occurring with nearby galaxies.
