This galaxy presents a roughly elliptical morphology, appearing somewhat amorphous with no clear spiral arm structure visible. The central region is significantly brighter and more concentrated, exhibiting a bluish-white color, indicative of potentially hotter, younger stellar populations. A fainter, greenish-blue halo surrounds the core, suggesting a lower density of stars or perhaps ionized gas emission. The outer edges of the halo fade into the background, implying a gradual decrease in stellar density or a truncation of the galaxy's extent. There is a slight asymmetry in the halo’s distribution, possibly due to minor gravitational interactions or internal dynamics. Overall, the galaxy seems to be an actively star-forming object, with potential signs of past or ongoing disturbances.
