The galaxy presents a generally smooth morphology, appearing largely elliptical in shape, though not perfectly rounded. There is some minor elongation evident. A central bulge region is visible, brighter and more concentrated, with a yellowish-orange hue, possibly indicating an older stellar population. The outer regions of the galaxy exhibit a slightly bluer tint, potentially suggestive of younger stars or ongoing, low-level star formation, though this is not prominently displayed. There is no obvious spiral structure or dust lane visible in this image. The overall impression is of a relatively quiescent galaxy. There is no visual indication of major mergers or significant tidal disturbances affecting its structure.
