This galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The light profile suggests a centrally dominant spheroid component. The overall color is yellowish-white, indicative of an older stellar population, possibly with ongoing low levels of star formation. The galaxy exhibits a slight elongation, not perfectly spherical, but rather somewhat "in between". There is no strong evidence of spiral arm structure or significant dust lanes visible in this image, nor is there indication of a major merger, though some minor disturbance cannot be ruled out.
