The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated light profile, with a gradual decrease in luminosity moving outward from the core. There is no discernable spiral arm structure or significant dust lane features visible. The galaxy possesses a rounded morphology with no signs of strong tidal disturbances or ongoing major mergers. Faint blue colors suggest some ongoing star formation, though the galaxy is mostly comprised of older stellar populations.
