The galaxy appears as a relatively smooth, elliptical structure with a dominant central bulge. It exhibits a concentrated, round morphology. There is some indication of a slight color gradient, transitioning from a bluer core to a redder outer region. The overall structure suggests an evolved system with a likely suppressed star formation rate. There is no clear evidence of spiral arms or significant dust lanes. The galaxy does not show signs of any major mergers or tidal disturbances. The absence of strong star formation regions, indicated by the lack of bright, blue knots, suggests that the galaxy is currently not undergoing significant star formation.
