The galaxy appears as a centrally concentrated object with a largely smooth morphology. It exhibits a moderately elliptical shape, appearing somewhat rounded but not perfectly spherical. The color gradient suggests an older stellar population, with the central region appearing slightly bluer relative to its outer regions, which suggests that the central region may still be forming stars. There's no obvious indication of spiral arm structure or a prominent disk. There are no visual signs of any ongoing major mergers or significant tidal disturbances. The galaxy shows a consistent color profile across its visible extent, without strong, localized color variations that would indicate dust lanes or localized bursts of star formation in the outer regions. Overall, the galaxy presents as a relatively quiescent system.
