The galaxy presents as a somewhat elliptical, smooth structure. The central bulge is a prominent, bright yellowish color suggesting an older stellar population with fewer young, massive stars. Moving outward from the core, the galaxy exhibits a gradual decrease in luminosity. There's a subtle color gradient shifting toward redder hues in the outer regions, further indicating older star populations. The overall shape appears regular and shows no distinct signs of active star formation regions or major disturbances. There may be some minor disturbances on the edges of the galaxy but this is indistinct. Based on these characteristics, the galaxy is likely a relatively massive elliptical galaxy with a modest ongoing star formation rate.
