The galaxy presents a relatively smooth, centrally concentrated morphology, appearing elliptical in shape, with a slight deviation from perfect circularity. The light profile suggests a mostly featureless structure, lacking prominent spiral arms or a distinct bar. The color gradient transitions from a redder hue towards the center, likely indicating an older stellar population concentrated in the galactic core, to a bluer, more diffuse halo. This halo component might be composed of younger stars or a more metal-poor population. There are hints of minor disturbances in the galaxy's structure, possibly from a past interaction or minor merger event, but these are not pronounced. The absence of strong dust lanes further contributes to its overall smooth and settled appearance. The color distribution and smooth structure are indicative of a relatively evolved galaxy with a low star formation rate.
