The galaxy presents a generally smooth morphology, appearing elliptical in shape. It exhibits a concentration of luminosity toward its center. The color profile suggests a redder core, transitioning to slightly bluer hues in the outer regions. There is no obvious evidence of spiral arm structure or significant dust lanes. The overall appearance is consistent with a galaxy dominated by an older stellar population, but with some ongoing star formation. There are no visible signs of a major merger event, although minor disturbances cannot be ruled out. The galaxy appears fairly isolated.