The galaxy presents as a centrally concentrated, relatively smooth object with a noticeable bulge. It appears elliptical in morphology, exhibiting a high degree of circularity. The galaxy's core is characterized by a bright, yellowish hue, suggesting an older stellar population. There is a subtle color gradient from the core to the outer regions. The outer regions exhibit a fainter and slightly bluer color, possibly indicative of younger stars or ongoing star formation, albeit at a low rate. There is no apparent spiral structure or significant tidal features. Overall, the galaxy appears as a relaxed system, showing no signs of recent major mergers or significant disturbances.
