The galaxy presents an overall elliptical morphology, appearing significantly elongated in shape, with a smooth light distribution. The central bulge region exhibits a reddish-orange hue, suggestive of an older stellar population dominated by red giants and a diminished rate of star formation. Fainter, greenish emissions extend outward from the bulge, possibly indicating the presence of ionized gas or regions of modest star formation activity. There's little evidence of spiral arm structure or significant dust lanes. The galaxy appears relatively undisturbed, with no obvious signs of ongoing mergers or tidal interactions. The overall appearance suggests a galaxy transitioning towards a more passive evolutionary state.
