The galaxy presents as a relatively smooth, elliptical morphology. The central bulge is prominent and appears to be composed of older stellar populations, inferred from its yellowish-orange color. There is a faint, diffuse halo surrounding the bulge, which seems to transition into a less structured, extended component on the left side of the image. There is little evidence of spiral arm structure or significant dust lanes. The galaxy shows no signs of major mergers or tidal disturbances, although there may be a very minor asymmetry or extension in the halo that might indicate a past interaction or accretion event. Overall, the galaxy appears to be a relatively evolved, quiescent system.
