This galaxy appears to be a relatively smooth, centrally concentrated object. The light distribution suggests a bulge-dominated system. The central region exhibits a yellowish hue, possibly indicating an older stellar population, whilst the outer regions of the galaxy present a bluer tinge, possibly indicating younger stars. The overall morphology suggests a galaxy that may be evolving into an elliptical galaxy, or a spiral galaxy with prominent bulge. There is no clear indication of spiral arm structure or significant dust lanes. There are no visible major disturbances.