The galaxy appears as a centrally concentrated object with a predominantly smooth morphology. The overall shape is roughly round, with only slight deviations from perfect circularity. There is a distinct central bulge, brighter and more condensed than the surrounding disk. Faint spiral arm structures might be present but are difficult to discern due to the overall smoothness and limited resolution. There are subtle color variations across the galaxy; the core region exhibits a redder hue, potentially indicative of an older stellar population, while the outer regions appear bluer, suggesting ongoing or recent star formation. There are no prominent dust lanes or signs of major disturbances, although a subtle asymmetry hints at a possible past minor interaction. Overall, this galaxy presents characteristics consistent with a relatively evolved spiral or an early-type galaxy transitioning to a more quiescent state.
