The galaxy presents an elongated, cigar-shaped morphology, indicative of an elliptical galaxy or a spiral galaxy viewed edge-on. Its light is distributed relatively smoothly, with the central region appearing brighter and more concentrated. The color gradient suggests a population of older stars dominating the central bulge, exhibiting a yellowish hue. Fainter, bluer regions are present along the galaxy's periphery, possibly representing areas of more recent, although subdued, star formation or a sparse spiral disk component. There is no obvious evidence of active galactic nuclei activity, major mergers, or significant tidal disturbances. The general structure points to a relatively quiescent galaxy that has likely undergone significant evolutionary processes.
